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Статті в журналах з теми "SLR parser"

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Автор: Grafiati

Опубліковано: 10 грудня 2022

Оновлено: 29 січня 2023

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1

Bhat, Spurthi, Rutuja Bhirud, and Vaishnavi Bhokare. "Survey on Various Syntax Analyzer Tools." International Journal for Research in Applied Science and Engineering Technology 10, no. 9 (September 30, 2022): 109–15. http://dx.doi.org/10.22214/ijraset.2022.46588.

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Abstract: Syntax analysis forms the second phase of a compiler. Syntax Analyzer basically takes the input of tokens from the lexical analyzer and parses the source code according to the production rules to detect errors in the code. The syntax analyzer gives an output in the form of a parse tree. The syntax analysis techniques can be classified as top-down parsing and bottom-up parsing. These categories can be further subdivided into recursive descent, LL (1), operator precedence, LR (0), SLR (1), CLR (1) and LALR (1) respectively. Various parser generators can generate parsers of these types which have been studied and analyzed in this paper such as Beaver, Tatoo, APG etc. This paper provides an overview of all these tools with respective to their working, advantages and features. These syntax analyzer tools can be used for different purposes according to the user.

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2

Khuri, Sami, and Jason Williams. "Understanding the bottom-up SLR parser." ACM SIGCSE Bulletin 26, no. 1 (March 12, 1994): 339–43. http://dx.doi.org/10.1145/191033.191163.

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3

Bermudez, Manuel E., Richard Newman-Wolfe, and George Logothetis. "Parallel construction of SLR (1) and LALR (1) parsers." International Journal of Parallel Programming 19, no. 3 (June 1990): 163–84. http://dx.doi.org/10.1007/bf01407953.

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4

Richard J. Golsan and James Golsan. "Interview With Robert Parker." South Central Review 27, no. 1-2 (2010): 163–66. http://dx.doi.org/10.1353/scr.0.0068.

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5

Speer, Roderick, and Kim Nielsen. "'Gallant Parker! Glory and Greece!': Lord Byron and Captain Sir Peter Parker." Byron Journal 36, no. 1 (June 2008): 57–62. http://dx.doi.org/10.3828/bj.36.1.7.

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6

Michaelson, Greg. "Implementing Prolog Definite Clause Grammars with SLR(1) parsers on the Relational Algebra Accelerator." Information and Software Technology 37, no. 10 (January 1995): 547–55. http://dx.doi.org/10.1016/0950-5849(95)90930-s.

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7

Kakabadse, Andrew. "An interview with Sir John Parker, Chairman, National Grid." Journal of Management Development 26, no. 4 (April 17, 2007): 381–88. http://dx.doi.org/10.1108/02621710710740129.

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8

Kay, Magdalena. "Miłosz: A Biography. By Andrzej Franaszek. Ed. and trans. Aleksandra and Michael Parker. Cambridge, Mass.: Belknap Press of Harvard University Press, 2017. 526 pp. Chronology. Notes. Bibliography. Index. Photographs. Maps. $35.00, hard bound." Slavic Review 77, no. 2 (2018): 506–7. http://dx.doi.org/10.1017/slr.2018.153.

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9

Menten, Karl M., and Mark J. Reid. "SiO and H2O Masers in the Central Parsec of the Galaxy." International Astronomical Union Colloquium 164 (1998): 229–30. http://dx.doi.org/10.1017/s0252921100045334.

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AbstractWe have discovered maser emission from SiO and H2O molecules toward a number of evolved stars within the central parsec of our Galaxy. The maser positions can be registered with milliarcsecond precision relative to the radio continuum emission of the nonthermal Galactic center source Sgr A*. Since the masing stars are prominent infrared sources, our data can be used to locate the position of Sgr A* on infrared images of the Galactic center region. Using VLBA observations it will be possible to measure proper motions of the maser stars, which can be used to put constraints on the mass distribution in the central parsec.

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10

Chen, Xian. "Sculpting the central parsec of our Galaxy." Proceedings of the International Astronomical Union 10, S312 (August 2014): 126–27. http://dx.doi.org/10.1017/s174392131500767x.

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AbstractRecent observations have revealed various structures within the gravitational influence of Sgr A* – the massive black hole in the Galactic center. These structures apparently defy the fundamental principles of star formation and stellar dynamics. On one hand, the red giants display a flat density profile, contrary to the cuspy one predicted by conventional stellar relaxation. On the other, Wolf-Rayet and OB stars are observed where in-situ star formation should have been prohibited by the strong tidal force from Sgr A*, and their spatial and phase-space distributions also contradict our understanding of stellar dynamics. To explain each of these inconsistencies, many scenarios have been proposed, which render the model increasingly complicated. Here, we suggest that the sub-parsec stellar disk surrounding Sgr A*, which was recently discovered, can reconcile all the above inconsistencies. We show that during the fragmenting past of this disk, the star-forming clumps could efficiently deplete red giants by repeatedly colliding with them. We also show that because of the torque exerted by the disk, stars within the central arcsec from Sgr A* would quickly mix in the angular-momentum space, which naturally explains the observed distributions of Wolf-Rayet and OB stars. Our results imply that Sgr A* was fueled by gas and stars several millions years ago and could have been an energetic AGN. We discuss future observations that can further testify our model.

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11

Moultaka, J., A. Eckart, K. Mužić, and N. Sabha. "A 3-D mid-infrared view of the central parsec." Proceedings of the International Astronomical Union 9, S303 (October 2013): 199–201. http://dx.doi.org/10.1017/s1743921314000556.

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AbstractWe present a mid-infrared 3D view of the central parsec using ISAAC spectrograph (ESO/VLT) with its spectroscopic mode. We mapped the central parsec in L- and M-bands by using 27 and 21 slit positions, respectively, that allowed us to build two data cubes of the region in these spectral domains. We also use an original method to distinguish the contribution of the foreground extinction to the absorbed spectra from that of the local extinction in both wavelength ranges. We find that there are residual water and CO ices in the central parsec as well as hydrocarbons and gaseous CO implying very low temperatures of the order of tens of Kelvin in the local environment of Sgr A*.

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12

Todd, Peyton. "ASL ‘topics’ revisited." Sign Language and Linguistics 11, no. 2 (August 21, 2009): 184–239. http://dx.doi.org/10.1075/sll.11.2.03tod.

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Sign linguists routinely parse ASL sentences using the category ‘topic’, by which is meant a constituent on the left edge of the main clause, structurally separate from it, and marked by a discrete formal symbolic event, more fully brow raise + backward head tilt + pause, although brow raise is sometimes considered sufficient. This paper provides evidence confirming suspicions that these left-detached constituents need not be marked by brow raise, and suggests that brow raise is better regarded as signaling a type of momentary focus — thus explaining why sign languages tend to employ it as they do — and that it belongs to a larger set of ‘topic-marking’ devices whose iconicity remains active in day-to-day signing.

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13

Armitage, David. "1320, 1776 and All That: A Tale of Two ‘Declarations’." Scottish Historical Review 101, no. 3 (December 2022): 512–31. http://dx.doi.org/10.3366/shr.2022.0581.

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Founding documents are parsed, revered and preserved but they can also be misread, mythologised and overlooked. This article examines the entangled fates of the Scots Declaration of Arbroath (1320) and the US Declaration of Independence (1776) at a moment between the seven-hundredth anniversary of the one in 2020 and the two-hundred-and-fiftieth anniversary of the other in 2026. It shows that the two ‘declarations’ were both diplomatic texts, rhetorically shaped, and part of sequences of similar documents that have otherwise been largely overlooked. Some recent commentators have suggested that Arbroath influenced the US Declaration; on the contrary, the article argues that the Declaration influenced Arbroath, at least in its reception and its construction as an alleged charter or ‘declaration’ of Scottish ‘independence’. I conclude by presenting fresh evidence for the presence of Arbroath in Philadelphia in 1776, to reflect on the sometimes surprising ways in which documents become, or do not become, foundational.

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14

Dantas, T. C. B. "Do Teatro ao Cinema: A Importância de Ser Prudente, de Oliver Parker." Revista Scripta Alumni, no. 5 (June 30, 2011): 98–110. http://dx.doi.org/10.18304/1984-6614/scripta.alumni.n5p98-110.

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15

Mafra, Janaína Silveira. "A postulação do ser e a recusa do poder ilimitado do discurso na primeira parte do Górgias de Platão." Nuntius Antiquus 2 (December 31, 2008): 72–89. http://dx.doi.org/10.17851/1983-3636.2..72-89.

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À partir du Gorgias de Platon, nous montrons que l'objet de la réfutation socratique est le discours, soit-il le produit des croyances de l'interlocuteur ou non, mais que le but de Socrate est principalement de conduire l’énonciateur refuté à se disposer effectivement à connaître quelque chose et à parler ou agir selon les déterminations de cette nouvelle connaissance.

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16

Coker, Robert F., and Sera Markoff. "Galactic Center: Implications of Recent Chandra Observations for Spherical Accretion Models of Sgr A*." Symposium - International Astronomical Union 205 (2001): 32–35. http://dx.doi.org/10.1017/s0074180900220342.

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At the center of the Milky Way lurks a unique compact nonthermal radio source, Sgr A*. It is thought to be powered by a 2.6 × 106 solar mass black hole that is accreting the stellar winds from the numerous early-type stars that exist in the central parsec. However, until recent high resolution Chandra observations, Sgr A* had never been unequivocably detected at wavelengths shorter than the sub-millimeter. We present a spherical accretion model which is consistent with both the flux and steep spectral shape of the X-ray emission from Sgr A*.

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17

Efthimiou, Eleni, Stavroula-Evita Fotinea, and Galini Sapountzaki. "Feature-based natural language processing for GSL synthesis." Sign Language and Linguistics 10, no. 1 (October 16, 2007): 3–23. http://dx.doi.org/10.1075/sll.10.1.03eft.

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The work reported in this study is based on research that has been carried out while developing a sign synthesis system for Greek Sign Language (GSL): theoretical linguistic analysis as well as lexicon and grammar resources derived from this analysis. We focus on the organisation of linguistic knowledge that initiates the multi-functional processing required to achieve sign generation performed by a virtual signer. In this context, structure rules and lexical coding support sign synthesis of GSL utterances, by exploitation of avatar technologies for the representation of the linguistic message. Sign generation involves two subsystems: a Greek-to-GSL conversion subsystem and a sign performance subsystem. The conversion subsystem matches input strings of written Greek-to-GSL structure patterns, exploiting Natural Language Processing (NLP) mechanisms. The sign performance subsystem uses parsed output of GSL structure patterns, enriched with sign-specific information, to activate a virtual signer for the performance of properly coded linguistic messages. Both the conversion and the synthesis procedure are based on adequately constructed electronic linguistic resources. Applicability of sign synthesis is demonstrated with the example of a Web-based prototype environment for GSL grammar teaching.

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18

Bosse, Kurt. "Indflydelse og medbestemmelse betaler sig — for begge parter." Tidsskrift for Arbejdsliv 7, no. 3 (September 1, 2005): 93. http://dx.doi.org/10.7146/tfa.v7i3.108501.

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Hvorfor er der så få arbejdsgivere, som har set det store ubrugte potentiale, der ligger i at give medarbejderne den nødvendige indflydelse? I denne artikel ser jeg nærmere på det gådefyldte fænomen, at arbejdsgivere har meget svært ved at lade medarbejderne på arbejdspladserne få indflydelse og medbestemmelse.

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19

Macquart, J. P., N. Kanekar, D. A. Frail, and S. M. Ransom. "A HIGH-FREQUENCY SEARCH FOR PULSARS WITHIN THE CENTRAL PARSEC OF Sgr A*." Astrophysical Journal 715, no. 2 (May 5, 2010): 939–46. http://dx.doi.org/10.1088/0004-637x/715/2/939.

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20

Mafra, Janaína Silveira. "A postulação do ser e a recusa do poder ilimitado do discurso na primeira parte do Górgias de Platão." Nuntius Antiquus 2 (December 31, 2008): 72. http://dx.doi.org/10.17851/1983-3636.2.0.72-89.

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<p>RÉSUMÉ</p> <p>À partir du Gorgias de Platon, nous montrons que l'objet de la réfutation socratique est le discours, soit-il le produit des croyances de l'interlocuteur ou non, mais que le but de Socrate est principalement de conduire l’énonciateur refuté à se disposer effectivement à connaître quelque chose et à parler ou agir selon les déterminations de cette nouvelle connaissance.</p> MOTS-CLÉS: élenkhos; réfutation; discours; connaissance; réalisation.

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21

Anderson, Gerald. "Peter Parker and the Introduction of Western Medicine in China Peter Parker et l'introduction de la médecine occidentale en Chine Peter Parker und die Einführung westlicher Medizin in China Peter Parker y la Introducción de Medicina Occidental en China." Mission Studies 23, no. 2 (2006): 203–38. http://dx.doi.org/10.1163/157338306778985776.

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AbstractIn the context of the life and missionary career of Peter Parker, M.D., a graduate of Yale who went to China in 1834, this article looks first at three issues: Who was the first medical missionary? Who was the first medical missionary in China? Who first introduced Western medicine in China?It also considers the tensions in the emerging understanding of the role of a medical missionary in the mid-nineteenth century, and the problems this caused for Parker, which led to his dismissal by the American Board of Commissioners for Foreign Missions.It then assesses the role of Parker as an American diplomat, when he became involved, first as a part-time secretary and interpreter, and confidential advisor, for the U.S. Commissioner to China, and helped to negotiate the first treaty between China and the United States in 1844. And later when Parker himself was appointed as the US Commissioner, and proposed aggressive military action against China, which led to his recall by the US State Department.Finally, in retirement for 30 years in Washington, DC, Parker received numerous honors and recognition, including appointment as a corporate member of the American Board, which earlier had terminated him as a missionary. Jetant un regard sur la vie et la carrière missionnaire de Peter Parker, M.D., diplômé de Yale parti en Chine en 1834, cet article pose d'abord trois questions: Qui a été le premier missionnaire médecin? Qui a été le premier missionnaire médecin en Chine? Qui a le premier introduit la médecine occidentale en Chine?Il considère aussi les tensions à l'œuvre dans la conception progressive du rôle d'un missionnaire médecin au milieu du dix-neuvième siècle, et les problèmes que cela a causé à Parker, allant jusqu'à la démission de ses fonctions par le Bureau américain des Missions étrangères.Il évalue ensuite le rôle de Parker comme diplomate américain lorsqu'il entra en scène d'abord comme secrétaire-interprète à temps partiel et conseiller particulier du Haut-commissaire américain pour la Chine, et qu'il aida à négocier le premier traité entre la Chine et les Etats-Unis en 1844. Et plus tard, lorsque Parker fut lui-même nommé Haut-commissaire américain et proposa une action militaire agressive contre la Chine, ce qui conduit à son rappel par le Département d'Etat américain.Finalement, retiré pendant trente ans à Washington, D.C., Parker reçut reconnaissance et de nombreux honneurs, y compris sa nomination au Bureau américain qui l'avait démis comme missionnaire quelques années auparavant. Im Zusammenhang mit dem Leben und der Missionslaufbahn des Arztes Peter Parker, einem Absolventen von Yale, der 1834 nach China ging, beleuchtet dieser Artikel eingangs drei Fragen: Wer war der erste ärztliche Missionar? Wer war der erste ärztliche Missionar in China? Wer hat die westliche Medizin als erster in China eingeführt?Der Artikel behandelt auch die Spannung zwischen dem damals entstehenden Begriff der Aufgabe eines ärztlichen Missionars Mitte des 19. Jahrhunderts und den Problemen, die er für Parker bedeutete und die zu seiner Entlassung vom American Board of Commissioners für auswärtige Mission führte.Dann bewertet der Artikel die Rolle Parkers als amerikanischer Diplomat, als er zuerst als Teilzeit Sekretär, Übersetzer und geheimer Berater für den US Commissioner in China arbeitete und ihm half, 1844 den ersten Vertrag zwischen China und den USA auszuhandeln. Und später, als Parker selbst zum US Commissioner bestellt wurde und eine aggressive militärische Vorgangsweise gegen China vorschlug, was zu seiner Abberufung durch das US State Department führte.Schließlich, über 30 Jahre im Ruhestand in Washington D.C., erhielt Parker zahlreiche Ehren und Anerkennung, eingeschlossen seine Berufung als Vollmitglied des American Board, das ihn früher als Missionar abgesetzt hatte. En el contexto de la vida y carrera misionera de Peter Parker, M.D., un graduado de la universidad Yale que fue a China en 1834, este artículo examina primero tres asuntos: ¿Quién era el primero misionero médico? ¿Quién era el primero misionero médico en China? ¿Quién era el primero para introducir medicina Occidental en China?También considera las tensiones en el entendimiento desallorrando del papel de un misionero médico en el siglo medio-decimonono, y los problemas éstas causó para Parker, que llevó a su despido por el Junta Norteamericano de Comisionados de las Misiones Extranjeras.Luego el articulo evalúa el papel de Parker como un diplomático norteamericano, cuando llegó a ser ocupado, primero como una secretaria de la jornada incompleta e intérprete, y consejero confidencial, para el EE.UU. Comisionado a China, y ayudó negociar el primer tratado entre China y los Estados Unidos en 1844. Y más tarde cuando Parker que se fijó como el Comisionado estadounidense, y se propuso acción agresiva militar contra China, que resultó en su revocación por el EE.UU. Departamento Estatal.Finalmente, durante su jubilación de 30 años en Washington, D.C., Parker recibió honores numerosos y reconocimiento, incluso su nombramiento como un miembro corporativo de la Junta Norteamericana, que más temprano lo había terminado como un misionero.

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22

Joyce, C. J., D. J. McComas, N. A. Schwadron, E. R. Christian, M. E. Wiedenbeck, R. L. McNutt, C. M. S. Cohen, et al. "Time evolution of stream interaction region energetic particle spectra in the inner heliosphere." Astronomy & Astrophysics 650 (June 2021): L5. http://dx.doi.org/10.1051/0004-6361/202039330.

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We analyze an energetic proton event associated with a stream interaction region (SIR) that was observed at Parker Solar Probe on day 320 of 2018 when the spacecraft was just 0.34 AU from the Sun. Using the Integrated Science Investigation of the Sun instrument suite, we perform a spectral analysis of the event and show how the observed spectra evolve over the course of the event. We find that the spectra from the first day of the event are much more consistent with local acceleration at a weak compression, while spectra from later on are more typical of SIR-related events in which particles accelerated at distant shocks dominate. After the first day, the spectra remain approximately constant, which indicates that the modulation of energetic particles during transit from the presumed source region is weaker than previously thought. We argue that these observations can be explained by a sub-Parker spiral magnetic field structure connecting the spacecraft to a source region in the SIR that is relatively close to the Sun. We further propose that acceleration at weak, pre-shock compressions likely plays an important role in observations of SIR-related events in the inner heliosphere and that future modelling of such events should consider acceleration all along the compression region, not just at the distant shock region.

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23

Czerny, Bozena, Vladimír Karas, Devaky Kunneriath, and Tapas K. Das. "Mini-spiral as source of material for Sgr A* in bright state." Proceedings of the International Astronomical Union 8, S290 (August 2012): 199–200. http://dx.doi.org/10.1017/s1743921312019606.

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AbstractThe question of the origin of the gas supplying the accretion process is pertinent especially in the context of enhanced activity of Galactic Center during the past few hundred years, seen now as echo from the surrounding molecular clouds, and the currently observed new cloud approaching Sgr A*. We discuss the so-called Galactic Center mini-spiral as a possible source of material feeding the supermassive black hole on a 0.1 parsec scale. The collisions between individual clumps reduce their angular momentum. and set some of the clumps on a plunging trajectory.We conclude that the amount of material contained in the mini-spiral is sufficient to sustain the luminosity of Sgr A* at the required level. The accretion episodes of relatively dense gas from the mini-spiral passing through a transient ring mode at ~ 104 Rg provide a viable scenario for the bright phase of Galactic Center.

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24

Clotet, Joaquim. "Bioética empírica e moral craft." Revista Bioética 29, no. 1 (March 2021): 27–35. http://dx.doi.org/10.1590/1983-80422021291443.

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Resumo Neste ensaio são examinados os conceitos de bioética empírica e moral craft segundo Michael Parker. A bioética fundamentada em princípios puramente teóricos mostra-se incapaz de resolver adequadamente conflitos de cunho ético, e a moral só pode ser compreendida no contexto real em que as pessoas vivem. Ambos os axiomas motivam, entre outros, o surgimento da bioética empírica, fundamentada em dados etnográficos, demográficos, de ciências sociais e empíricos. Trata-se de aprender e de resolver conflitos por meio do exercício diário, dos êxitos e erros, de soluções que foram adquiridas e validadas na prática. Moral craft é o conjunto de princípios e valores morais elaborado de forma individual ou coletiva, imprescindíveis para a análise, o estudo e a pesquisa de um caso ou problema. O moral craft como apresentado por Parker revela o caráter que aperfeiçoa a ética empirista.

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25

Andrade, Mariana Nunes, Rejane Santos, and Ivanete Batista dos Santos. "ELEMENTOS DE UMA MATEMÁTICA PARA ENSINAR: uma análise das orientações para ensinar aritmética referentes às Cartas de Parker (1902)." ACERVO - Boletim do Centro de Documentação do GHEMAT-SP 3 (October 16, 2021): 1–13. http://dx.doi.org/10.55928/acervo.2675-2646.2021.3.47.

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Анотація:

Neste texto é apresentado o resultado de uma pesquisa que teve por objetivo caracterizar elementos de uma matemática para ensinar a partir de orientações das Cartas de Parker. Para uma aproximação com o tema foi adotado Valente (2008, 2013, 2018 e 2019) para compreender sobre a história da educação matemática, sobre as Cartas de Parker e sobre o saber profissional do professor que ensina matemática e Maciel (2019) que trata também sobre os saberes profissionais do professor que ensina matemática. Por meio do exame realizado em artigos da Revista de Ensino, acerca das Cartas, identificar elementos de uma aritmética para ensinar, os quais indicam o uso de objetos concretos e uma ordem para o ensino a ser seguida, saindo do concreto para chegar ao abstrato, levando a classe a resolver o que está sendo proposto pelo professor.

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26

Bracci, Enrico, and Mouhcine Tallaki. "Socio-environmental reporting trends in the Italian local government: Thrive or wither?" FINANCIAL REPORTING, no. 2 (September 2013): 27–46. http://dx.doi.org/10.3280/fr2013-002003.

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Анотація:

Social and environmental reporting (SER) in the public sector has been widelydiscussed in the last years (Gray et al., 1996; Mathews, 1997; Parker 2005; Guthrieand Abeysekera, 2006; Guarini, 2002; Hinna 2004; Marcuccio and Steccolini,2005). However, despite the interest in this area of research, there are still a numberof calls to deepen the study of SER in the public sector (Lewis, 2008; Grubnikand Ball, 2007). In Italy, the literature shows the risk of adopting SER as a managementfashion, more than a conscious process of organizational change (Marcuccioand Steccolini, 2005). This paper investigates about the reasons for theadoption and eventual abandonment of SER by local government in Italy.

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27

Russell, Christopher M. P., Q. Daniel Wang, and Jorge Cuadra. "Modelling the thermal X-ray emission around the Galactic centre from colliding Wolf-Rayet winds." Proceedings of the International Astronomical Union 12, S329 (November 2016): 443. http://dx.doi.org/10.1017/s1743921317003131.

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AbstractWe compute the thermal X-ray emission from hydrodynamic simulations of the 30 Wolf-Rayet (WR) stars orbiting within a parsec of Sgr A*, with the aim of interpreting the Chandra X-ray observations of this region. The model well reproduces the spectral shape of the observations, indicating that the shocked WR winds are the dominant source of this thermal emission. The model X-ray flux is tied to the strength of the Sgr A* outflow, which clears out hot gas from the vicinity of Sgr A*. A moderate outflow best fits the present-day observations, even though this supermassive black hole (SMBH) outflow ended ~100 yr ago.

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28

Yusef-Zadeh, F., R. Arendt, H. Bushouse, W. Cotton, D. Haggard, M. W. Pound, D. A. Roberts, M. Royster, and M. Wardle. "ERRATUM: “A THREE PARSEC-SCALE JET-DRIVEN OUTFLOW FROM Sgr A*” (2012, ApJL, 758, L11)." Astrophysical Journal 777, no. 2 (October 25, 2013): L39. http://dx.doi.org/10.1088/2041-8205/777/2/l39.

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29

Sabha, N., M. Zamaninasab, A. Eckart, and L. Moser. "A new MIR bow shock source in the Galactic center." Proceedings of the International Astronomical Union 9, S303 (October 2013): 150–52. http://dx.doi.org/10.1017/s1743921314000428.

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AbstractWe find a convex-like feature at a distance of 0.68 pc (17″) from the position of the supermassive black hole, Sgr A*, at the center of the nuclear stellar cluster. This feature resembles a stellar bow shock with a symmetry axis pointing to the center. We discuss the possible nature of the feature and the implications of its alignment with other dusty comet-like objects inside the central parsec.

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30

Lucas, Peter J. "The earliest modern Anglo-Saxon grammar: Sir Henry Spelman, Abraham Wheelock and William Retchford." Anglo-Saxon England 45 (December 2016): 379–417. http://dx.doi.org/10.1017/s0263675100080339.

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AbstractThe first scholars interested in Anglo-Saxon had to learn it by direct contact with original sources. Work on a dictionary preceded that on a grammar, notably through the efforts of John Joscelyn, Archbishop Parker's Latin Secretary. Like Parker, Sir Henry Spelman (1563/4–1641) found that many of his sources for early English history were in Anglo-Saxon. Consequently he encouraged the study of Old English by establishing a Lectureship in Anglo-Saxon at Cambridge University and worked closely with its first (and only) holder, Abraham Wheelock. Together with Wheelock's pupil, William Retchford, and possibly drawing on some earlier work by Joscelyn (since lost), these scholars attempted to formulate the rudiments of Anglo-Saxon grammar. This pioneering work, basically a parts-of-speech grammar, survives in three versions, two of them incomplete. In this article I discuss the contents and methodology used and present for the first time an edited text of the first modern Old English grammar. It was a remarkable achievement.

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31

Souza, Sarah Nancy Deggau Hegeto de, Edilaine Giovanini Rossetto, and Thelma Malagutti Sodré. "Aplicação da teoria de Parse no relacionamento enfermeiro-indivíduo." Revista da Escola de Enfermagem da USP 34, no. 3 (September 2000): 244–51. http://dx.doi.org/10.1590/s0080-62342000000300004.

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O estudo tem o objetivo de relatar experiências de situações vividas pelas autoras ao aplicarem os fundamentos da teoria de Parse "Human Becoming" e apresentar seus princípios e conceitos visando divulgá-la. Após estudo teórico para a compreensão da teoria, os seus princípios foram aplicados na prática. As autoras constataram que isto implica em mudança de valores e crenças do enfermeiro, transformando sua visão sobre o ser humano e sua saúde, tornando o cuidado mais humanístico. A experiência vivenciada possibilitou amadurecimento pessoal e profissional das autoras.

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32

Moser, Lydia, Álvaro Sánchez-Monge, Andreas Eckart, Miguel A. Requena-Torres, Macarena García-Marin, Devaky Kunneriath, Anton Zensus, et al. "Molecular gas in the immediate vicinity of Sgr A* seen with ALMA." Proceedings of the International Astronomical Union 11, S322 (July 2016): 129–32. http://dx.doi.org/10.1017/s1743921316012126.

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AbstractWe report serendipitous detections of line emission with ALMA in band 3, 6, and 7 in the central parsec of the Galactic center at an up to now highest resolution (<0.7″). Among the highlights are the very first and highly resolved images of sub-mm molecular emission of CS, H13CO+, HC3N, SiO, SO, C2H, and CH3OH in the immediate vicinity (~1″ in projection) of Sgr A* and in the circumnuclear disk (CND). The central association (CA) of molecular clouds shows three times higher CS/X (X: any other observed molecule) luminosity ratios than the CND suggesting a combination of higher excitation - by a temperature gradient and/or IR-pumping - and abundance enhancement due to UV- and/or X-ray emission. We conclude that the CA is closer to the center than the CND is and could be an infalling clump consisting of denser cloud cores embedded in diffuse gas. Moreover, we identified further regions in and outside the CND that are ideally suited for future studies in the scope of hot/cold core and extreme PDR/XDR chemistry and consequent star formation in the central few parsecs.

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33

Habing, H. J. "Stellar Populations in the Galactic Bulge." Symposium - International Astronomical Union 169 (1996): 317–27. http://dx.doi.org/10.1017/s0074180900229859.

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In this review I discuss stars in the bulge of our Milky Way, but I exclude stars within a few parsec from Sgr A West; they are the subject of other reviews at this Symposium. We should, however, not forget that there may be an intimate connection between the central cluster and the bulge: bulge stars may eject matter that feeds the monster at the center and eruptions by this monster may have an important effect on the bulge.

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34

Lawrence, Robert G. "John Ripley ed. Gilbert Parker and Herbert Beerbohm Tree Stage 'The Seats of the Mighty'John Coldwell Adams, Seated with the Mighty: A Biography of Sir Gilbert Parker." Theatre Research in Canada 9, no. 2 (January 1988): 207–10. http://dx.doi.org/10.3138/tric.9.2.207.

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35

Goto, Miwa. "The cosmic ray ionization rate in the central parsec of the Galaxy." Proceedings of the International Astronomical Union 9, S303 (October 2013): 429–33. http://dx.doi.org/10.1017/s1743921314001070.

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AbstractCosmic rays represent a unique crossing point of high-energy astrophysics and astrochemistry. The cosmic ray ionization rate of molecular hydrogen (ζ2) measured by H3+ spectroscopy in the central parsec of the Galaxy is 2 orders of magnitude higher than that in the dense clouds outside the Galactic center. However, it is still too short, by the factor of 10,000, to agree with an extremely high ζ2 that accommodates the new γ-ray observations of Sgr A* and its environment.

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36

Eckart, A., R. Genzel, R. Hofmann, B. J. Sams, and L. E. Tacconi-Garman. "Diffraction Limited Near Infrared Imaging of the Central Parsec of the Galaxy." Symposium - International Astronomical Union 158 (1994): 379–81. http://dx.doi.org/10.1017/s0074180900107983.

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We present deep 1.6 and 2.2 μm images of the central parsec of the Galaxy at a resolution of 0.15″. Most of the flux in earlier seeing limited images comes from about 340 unresolved stellar sources with K≤14. The IRS 16 and 13 complexes are resolved into about two dozen and half a dozen sources, a number of which are probably luminous hot stars. We confirm the presence of a blue near infrared object (K≈13) at the position of the compact radio source Sgr A∗. The spatial centroid of the source number distribution is consistent with the position of Sgr A∗ but not with a position in the IRS 16 complex. The stellar surface density in the central 10″ is very well fitted by an isothermal cluster model with a well defined core radius. The derived core radius of all 340 sources is 0.15±0.05 pc. The central stellar density is a few times 107 M⊙ pc−3. Buildup of massive stars by merging of lower mass stars and collisional disruption of giant atmospheres are very probable processes in the central 0.2 pc.

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37

Everill, Paul. "The Parkers of Heytesbury: Archaeological Pioneers." Antiquaries Journal 90 (September 2010): 441–53. http://dx.doi.org/10.1017/s000358151000003x.

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AbstractThis paper uses original documentary evidence held in the archives of the Wiltshire Archaeological and Natural History Society in Devizes to reassess the work of William Cunnington, FSA, carried out on behalf of Sir Richard Colt Hoare, and the contribution of his two principal excavators, Stephen and John Parker, of Heytesbury, in Wiltshire. Previously the Parkers have been regarded as little more than regular labourers on Cunnington’s pioneering excavations; the evidence now suggests that they (and in particular John) were, in fact, key to the success of Cunnington’s work. By the time of Cunnington’s death in 1810, John Parker was identifying new sites on the Wiltshire Downs and, on occasion, taking sole responsibility for excavating and interpreting them. After 1810 Hoare sponsored few further excavations and, though John was employed on at least one occasion, in 1814, the Parkers dropped back into obscurity and poverty without the regular employment, and perhaps protection, provided by Cunnington. Although John’s obituary in 1867 described him as Cunnington’s ‘principal pioneer’, no research has previously been undertaken that specifically considers the contribution of the Parkers in those early British excavations. This paper seeks to redress that oversight.

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38

Bellegarda, J. R., and D. C. Farden. "Comments, with reply, on "A new efficient adaptive cascade lattice structure" by M. Tummala and S.R. Parker." IEEE Transactions on Circuits and Systems 37, no. 6 (June 1990): 858–60. http://dx.doi.org/10.1109/31.55054.

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39

SILVA, C. A., G. SANTILLI, E. E. SANO, and S. W. P. RODRIGUES. "Qualitative Analysis of Deforestation in the Amazonian Rainforest from SAR, Optical and Thermal Sensors." Anuário do Instituto de Geociências - UFRJ 42, no. 4 (December 12, 2019): 18–29. http://dx.doi.org/10.11137/2019_4_18_29.

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40

Coker, Robert, and Fulvio Melia. "7.14. Gaseous accretion flows in the inner parsec of the Galaxy." Symposium - International Astronomical Union 184 (1998): 319–20. http://dx.doi.org/10.1017/s0074180900085107.

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Many characteristics of galactic nuclei may be associated with the accretion of ambient gas by a central concentration of mass. Using a 3D hydrodynamical code, we have been simulating this accretion process for Sgr A∗, the compact nonthermal source at the center of the Milky Way, in order to realistically model the gaseous flows in the inner parsec of our Galaxy. In the most recent simulations, we have taken into account the multi-point-like distribution of wind sources and we find that the structure of the flow can be significantly different from that due to a uniform medium. We here present our results concerning the mass and angular momentum accretion rates and discuss how these may be used to set constraints on our Galaxy's central engine.

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41

Pereira, Valdete Preve, and Miriam Süsskind Borenstein. "Iluminando as vivências de mulheres portadoras de transtornos psíquicos e moradoras de uma residência terapêutica." Texto & Contexto - Enfermagem 13, no. 4 (December 2004): 527–34. http://dx.doi.org/10.1590/s0104-07072004000400004.

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Trata-se de estudo com abordagem qualitativa, cujo objetivo é refletir com mulheres portadoras de transtornos psíquicos, o vivenciar de seu cotidiano, identificando os significados e co-construindo possibilidades de "vir-a-ser mais" como cidadãs. O estudo foi desenvolvido com moradoras de uma Residência Terapêutica, vinculada ao Instituto de Psiquiatria de Santa Catarina, em São José/SC. A coleta dos dados efetivou-se concomitante à implementação do processo de cuidado, segundo a teoria de Parse. Na análise dos dados foram identificados os seguintes significados: convivendo com o transtorno psíquico; co-constituindo padrões de inter-relação com outros; convivendo com as dificuldades de enfrentamento e superação de limites; co-criando possibilidades de vir-a-ser em saúde, cidadania e qualidade de vida; e co-construindo a Residência Terapêutica como espaço de reabilitação psicossocial. Concluiu-se que vivenciar este processo propiciou mudanças de perspectivas destas mulheres, contribuindo para a mobilização de transcendências, no sentido de "vir-a-ser mais" como ser humano.

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42

Sperandio, Natália Elvira, and Antônio Luiz Assunção. "Pensando a metáfora por um viés cognitivo e cultural." Revele: Revista Virtual dos Estudantes de Letras 3 (December 31, 2011): 183. http://dx.doi.org/10.17851/2317-4242.3.0.183-198.

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Quando analisamos o percurso histórico dos estudos dedicados à metáfora percebemosque grandes mudanças ocorreram na forma de conceituá-la, deixando de ser vista comoapenas uma forma de embelezar discursos especiais, como, por exemplo, o poético; paraser considerada uma importante figura de pensamento, onipresente não apenas emnossa linguagem, mas em nossas ações e pensamentos. Diante dessas mudanças, opresente artigo tem por finalidade fazer uma revisão de literatura acerca da evoluçãoocorrida nos estudos dedicados à metáfora nas últimas décadas. Para isso,apresentaremos um percurso histórico das principais teorias que têm se dedicado aoestudo da metáfora, com destaque para aquelas que a concebem como processocognitivo e cultural.

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43

HOPPER, ANDREW J. "Savage Fortune: An Aristocratic Family in the Early Seventeenth Century Edited by Lyn Boothman and Sir Richard Hyde Parker." History 92, no. 307 (July 2007): 396–97. http://dx.doi.org/10.1111/j.1468-229x.2007.401_31.x.

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44

De Mello, Thaís Lisboa Roussille Bandeira, and Valéria Regina Zanetti. ""BONNIE E CLYDE”: UMA ANÁLISE EM DOIS TEMPOS (1967-2013)." Revista Univap 22, no. 40 (April 17, 2017): 763. http://dx.doi.org/10.18066/revistaunivap.v22i40.1559.

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Este trabalho tem a finalidade de apresentar uma breve análise a respeito de dois filmes lançados sobre a história do casal de gangsteres Bonnie Parker e Clyde Barrow.que atuaram na região do Texas, Estados Unidos durante a década de 1930, assim como suas diferenças e semelhanças com a história verdadeira do casal. O primeiro filme a ser analisado, “Bonnie e Clyde- Uma Rajada de Balas” (1967), e o segundo a minissérie para TV “Bonnie & Clyde” (2013), apresentam a carreira, assim como a popularidade, do casal de formas diferentes, gerando questionamentos a respeito de sua veracidade histórica, tema abordado no presente artigo a partir de análises de críticas e biografias escritas sobre os mesmos.

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45

Wardle, Mark, and Farhad Yusef-Zadeh. "The origin of Keplerian megamaser disks." Proceedings of the International Astronomical Union 8, S287 (January 2012): 354–55. http://dx.doi.org/10.1017/s1743921312007302.

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AbstractSeveral examples of thin, Keplerian, sub-parsec megamaser disks have been discovered in the nuclei of active galaxies and used to precisely determine the mass of their host black holes. We show that there is an empirical linear correlation between the disk radius and black hole mass and that such disks are naturally formed as molecular clouds pass through the galactic nucleus and temporarily engulf the central supermassive black hole. For initial cloud column densities below about 1023.5 cm−2 the disk is non-self gravitating, but for higher cloud columns the disk would fragment and produce a compact stellar disk similar to that observed around Sgr A* at the galactic centre.

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46

Lucas, William, Ian Bonnell, Melvyn Davies, and Ken Rice. "Forming misaligned stellar disks around a massive black hole: cloud infall in the Galactic center." Proceedings of the International Astronomical Union 9, S303 (October 2013): 245–47. http://dx.doi.org/10.1017/s1743921314000672.

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AbstractThe innermost parsec around Sgr A* has been found to play host to two disks or streamers of O and W-R stars. They are misaligned by an angle approaching 90°. That the stars are approximately coeval indicates that they formed in the same event rather than independently. We have performed smoothed particle hydrodynamic simulations of the infall of a single prolate cloud towards a massive black hole. As the cloud is disrupted, the large spread in angular momentum can, if conditions allow, lead to the creation of misaligned gas disks. In turn, stars may form within those disks. We are now investigating the origins of these clouds in the Galactic center (GC) region.

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47

Liu, Wei, Jian Wang, Jiancheng Luo, Zhifeng Wu, Jingdong Chen, Yanan Zhou, Yingwei Sun, Zhanfeng Shen, Nan Xu, and Yingpin Yang. "Farmland Parcel Mapping in Mountain Areas Using Time-Series SAR Data and VHR Optical Images." Remote Sensing 12, no. 22 (November 13, 2020): 3733. http://dx.doi.org/10.3390/rs12223733.

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Accurate, timely, and reliable farmland mapping is a prerequisite for agricultural management and environmental assessment in mountainous areas. However, in these areas, high spatial heterogeneity and diversified planting structures together generate various small farmland parcels with irregular shapes that are difficult to accurately delineate. In addition, the absence of optical data caused by the cloudy and rainy climate impedes the use of time-series optical data to distinguish farmland from other land use types. Automatic delineation of farmland parcels in mountain areas is still a very difficult task. This paper proposes an innovative precise farmland parcel extraction approach supported by very high resolution(VHR) optical image and time series synthetic aperture radar(SAR) data. Firstly, Google satellite imagery with a spatial resolution of 0.55 m was used for delineating the boundaries of ground parcel objects in mountainous areas by a hierarchical extraction scheme. This scheme divides farmland into four types based on the morphological features presented in optical imagery, and designs different extraction models to produce each farmland type, respectively. The potential farmland parcel distribution map is then obtained by the layered recombination of these four farmland types. Subsequently, the time profile of each parcel in this map was constructed by five radar variables from the Sentinel-1A dataset, and the time-series classification method was used to distinguish farmland parcels from other types. An experiment was carried out in the north of Guiyang City, Guizhou Province, Southwest China. The result shows that, the producer’s accuracy of farmland parcels obtained by the hierarchical scheme is increased by 7.39% to 96.38% compared with that without this scheme, and the time-series classification method produces an accuracy of 80.83% to further obtain the final overall accuracy of 96.05% for the farmland parcel maps, showing a good performance. In addition, through visual inspection, this method has a better suppression effect on background noise in mountainous areas, and the extracted farmland parcels are closer to the actual distribution of the ground farmland.

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48

Zhao, Jun-Hui, Mark R. Morris, and W. M. Goss. "Detection of a Dense Group of Hypercompact Radio Sources in the Central Parsec of the Galaxy." Astrophysical Journal Letters 927, no. 1 (March 1, 2022): L6. http://dx.doi.org/10.3847/2041-8213/ac54be.

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Abstract Using the JVLA, we explored the Galactic center (GC) with a resolution of 0.″05 at 33.0 and 44.6 GHz. We detected 64 hypercompact radio sources (HCRs) in the central parsec. The dense group of HCRs can be divided into three spectral types: 38 steep-spectrum (α ≤ −0.5) sources, 10 flat-spectrum (−0.5 < α ≤ 0.2) sources, and 17 inverted-spectrum sources having α > 0.2, assuming S ∝ ν α . The steep-spectrum HCRs are likely to represent a population of massive stellar remnants associated with nonthermal compact radio sources powered by neutron stars and stellar black holes. The surface-density distribution of the HCRs as a function of radial distance (R) from Sgr A* can be described as a steep power law Σ(R) ∝ R −Γ, with Γ = 1.6 ± 0.2, along with the presence of a localized order-of-magnitude enhancement in the range 0.1–0.3 pc. The steeper profile of the HCRs relative to that of the central cluster might result from the concentration of massive stellar remnants by mass segregation at the GC. The GC magnetar SGR J1745−2900 belongs to the inverted-spectrum subsample. We find two spectral components present in the averaged radio spectrum of SGR J1745−2900, separated at ν ∼ 30 GHz. The centimeter component is fitted to a power law with α cm = −1.5 ± 0.6. The enhanced millimeter component shows a rising spectrum α mm = 1.1 ± 0.2. Based on the ALMA observations at 225 GHz, we find that the GC magnetar is highly variable on a day-to-day timescale, showing variations up to a factor of 6. Further JVLA and ALMA observations of the variability, spectrum, and polarization of the HCRs are critical for determining whether they are associated with stellar remnants.

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49

Chhatkuli, D. N., S. Paudel, A. K. Gautam, and B. Aryal. "SDSS J114818.18-013823.7: Forming Compact Dwarf Galaxy through the Dwarf-Dwarf Merger." Journal of Nepal Physical Society 7, no. 2 (August 6, 2021): 49–57. http://dx.doi.org/10.3126/jnphyssoc.v7i2.38622.

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We studied the spectroscopic properties of the low redshift (z = 0.0130) interacting dwarf galaxy SDSS J114818.18-013823.7. It is a compact galaxy of half-light radius 521 parsec. It’s r-band absolute magnitude is -16.71 mag. Using a publicly available optical spectrum from the Sloan Sky Survey data archive, we calculated star-formation rate, emission line metallicity, and dust extinction of the galaxy. Star formation rate (SFR) due to Hα is found to be 0.118 Mʘ year-1 after extinction correction. The emission-line metallicity, 12+log(O/H), is 8.13 dex. Placing these values in the scaling relation of normal galaxies, we find that SDSS J114818.18-013823.7 is a significant outlier from both size-magnitude relation and SFR-B-band absolute relation. Although SDSS J114818.18-013823.7 possess enhance rate of star-formation, the current star-formation activity can persist several Giga years in the future at the current place and it remains compact.

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50

Nogueira, Conceição. "Construcionismo social, discurso e género." PSICOLOGIA 15, no. 1 (February 12, 2014): 43. http://dx.doi.org/10.17575/rpsicol.v15i1.490.

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Os desafios colocados no presente à psicologia, e nomeadamente à psicologia social, podem ser considerados como fazendo parte dos debates iniciados pelo pós-modernismo como corrente geral, mas que na psicologia social se organizam em torno da escola do “construcionismo social” (Gergen, 1994a; 1994b; Shotter, 1993, 1995), ou mesmo da “psicologia discursiva” (Harré, 1995; Harré & Gillett, 1994; Parker, 1992; Potter & Wetherell, 1987). Depois de sistematizados os pressupostos destas perspectivas e apresentada a emergência de novas realidades e recursos de acção, analisar-se-á como o género pode ser concebido nestas novas abordagens, no quadro de uma breve reflexão sobre a problemática do relativismo nestas perspectivas. Terminamos apresentando as alternativas e estratégicas necessárias a uma psicologia feminista, que tem pela frente um conjunto de questões que representam desafios estimulantes para o debate que urge continuar, sem esquecer a acção política, sempre necessária à construção da igualdade entre homens e mulheres.DOI: http://dx.doi.org/10.17575/rpsicol.v15i1.490

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