Relevant bibliographies by topics / Solar-type star

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  2. Dissertations / Theses
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  5. Conference papers

Academic literature on the topic 'Solar-type star'

Author: Grafiati
Published: 4 June 2021
Last updated: 19 February 2022

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Journal articles on the topic "Solar-type star"

1

Smith, Keith T. "Is the Sun a solar-type star?" Science 357, no. 6347 (2017): 159.1–159. http://dx.doi.org/10.1126/science.357.6347.159-a.

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Mirzoyan, L. V. "Flare stars in star clusters, associations and solar vicinity." Symposium - International Astronomical Union 137 (1990): 1–13. http://dx.doi.org/10.1017/s0074180900187303.

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The observational data on flare stars observed in star clusters and associations as well as in the solar vicinity (the UV Ceti type stars) are discussed. The analysis of these data show that they constitute one common class of objects possessing flare activity and the differences between them are conditioned by the age differences. The stage of flare activity is an evolutionary stage, one of the earliest stages of evolution passed by all red dwarf stars. It comes before the end of their T Tau stage of evolution. The UV Ceti type flare stars in the solar vicinity seem to be the population of th
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He, Han, Huaning Wang, Yan Yan, and Duo Yun. "Magnetic Activity Discrepancies of Solar-Type Stars Revealed by Kepler Light Curves." Proceedings of the International Astronomical Union 13, S335 (2017): 7–10. http://dx.doi.org/10.1017/s1743921317007670.

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AbstractMagnetic activity information is concealed in the shape of stellar light curves owing to the process of rotational modulation. We developed approaches to extract magnetic activity characteristics from stellar light curves, and applied the method to a solar-type star observed with Kepler space telescope and also to the Sun for comparison. The result reveals distinct magnetic activity discrepancies between the solar-type star and the Sun. (1) The light-curve periodicity of the solar-type star is generally stronger than that of the Sun. (2) For the solar-type star, when the range of light
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Roberts, Lewis C., Andrei Tokovinin, Brian D. Mason, William I. Hartkopf, and Reed L. Riddle. "OBSERVATIONS OF HIERARCHICAL SOLAR-TYPE MULTIPLE STAR SYSTEMS." Astronomical Journal 150, no. 4 (2015): 130. http://dx.doi.org/10.1088/0004-6256/150/4/130.

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Porto de Mello, G. F., and L. da Silva. "HR 6094: A Young Solar-Type, Solar-Metallicity Barium Dwarf Star." Astrophysical Journal 476, no. 2 (1997): L89—L92. http://dx.doi.org/10.1086/310504.

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da Silva, L., and G. F. Porto de Mello. "Lithium Abundances in Solar-Type Stars." Symposium - International Astronomical Union 198 (2000): 495–97. http://dx.doi.org/10.1017/s0074180900167142.

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We report Li abundances from the λ6707 line for 19 nearby dwarf and subgiant solar-type stars. The unevolved stars in this sample present high (> 2.00) Li abundances. We found a few cases of subgiant stars which present high Li content. The Sun seems to be part of a population of nearly unevolved stars which have depleted their Li to a high degree: all other metal-normal, near ZAMS stars in our sample show higher than solar Li content. There seems to be no correlation of the degree of Li depletion with mass, atmospheric parameters or state of evolution: as an example we found a star (HR1532
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Mayor, Michel, and Didier Queloz. "A Jupiter-mass companion to a solar-type star." Nature 378, no. 6555 (1995): 355–59. http://dx.doi.org/10.1038/378355a0.

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Soderblom, David R. "Determining the temperatures of solar-type stars - Do star spots produce color anomalies?" Astrophysical Journal 342 (July 1989): 823. http://dx.doi.org/10.1086/167639.

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Brown, Carolyn, Brad Carter, Stephen Marsden, and Ian Waite. "Starspots on Young Solar-Type Stars." Proceedings of the International Astronomical Union 9, S302 (2013): 148–49. http://dx.doi.org/10.1017/s1743921314001938.

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AbstractDoppler Imaging of starspots on young solar analogues is a way to investigate the early history of solar magnetic activity by proxy. Doppler images of young G-dwarfs have yielded the presence of large polar spots, extending to moderate latitudes, along with measurements of the surface differential rotation. The differential rotation measurement for one star (RX J0850.1-7554) suggests it is possibly the first example of a young G-type dwarf whose surface rotates as almost a solid body, in marked contrast to the differential rotation of other rapidly rotating young G-dwarfs and the prese
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Barker, Adrian J., and Gordon I. Ogilvie. "Internal wave breaking and the fate of planets around solar-type stars." Proceedings of the International Astronomical Union 6, S271 (2010): 363–64. http://dx.doi.org/10.1017/s1743921311017807.

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AbstractInternal gravity waves are excited at the interface of convection and radiation zones of a solar-type star, by the tidal forcing of a short-period planet. The fate of these waves as they approach the centre of the star depends on their amplitude. We discuss the results of numerical simulations of these waves approaching the centre of a star, and the resulting evolution of the spin of the central regions of the star and the orbit of the planet. If the waves break, we find efficient tidal dissipation, which is not present if the waves perfectly reflect from the centre. This highlights an
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Dissertations / Theses on the topic "Solar-type star"

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Al-Edhari, Ali Jaber. "Complex organic molecules in solar-type star forming regions." Thesis, Université Grenoble Alpes (ComUE), 2016. http://www.theses.fr/2016GREAY048/document.

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Le but de la présente thèse est l'étude de la compléxité moléculaire dans les régions de formation stellaires. Cette thèse s'axe sur deux classes de molécule aux caractéristiques prébiotiques : les molécules organiques complexes et les cyanopolyynes.Dans ce contexte, j'ai analysé des données d'un seul échantillon de relevés spec- traux en exploitant des codes de transfert radiatif à l'équilibre thermodynamique local (LTE) et/ou non-LTE pour deux sources : une proto-étoile de type solaire dans un environnement calme (IRAS 16293-2422) et un proto-ama constitué de proto-étoile de type solaire (OM
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Mengel, Matthew Wayne. "The active young solar-type star HR 1817 (=HD 35850)." University of Southern Queensland, Faculty of Sciences, 2005. http://eprints.usq.edu.au/archive/00001474/.

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The active F dwarf HR 1817 represents the upper temperature extreme of what are broadly termed solar-type stars - stars which have the same internal structure as the Sun, albeit in this case with a much smaller convective zone. To date, studies of the active surface features and magnetic fields of solar-type stars have been restricted to G and K dwarfs. This thesis investigates the surface and magnetic features of HR 1817 using the techniques of Doppler and Zeeman Doppler Imaging, resulting in tomographic maps of the stellar surface and magnetic field. Cooler stars than HR 1817 exhibit large p
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Namekata, Kousuke. "Observational Studies of Extreme Stellar Magnetic Activities: Spots, Flares, and Mass Ejections." Doctoral thesis, Kyoto University, 2021. http://hdl.handle.net/2433/263473.

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Fuentes, Pineda Rosinda. "Triphenylamine-based hole transport materials for perovskite solar cells." Thesis, University of Edinburgh, 2018. http://hdl.handle.net/1842/31410.

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The rapid development in perovskite solar cells (PSC) has generated a tremendous interest in the photovoltaic community. The power conversion efficiency (PCE) of these devices has increased from 3.8% in 2009 to a recent certified efficiency of over 20% which is mainly the product of the remarkable properties of the perovskite absorber material. One of the most important advances occurred with the replacement of the liquid electrolyte with a solid state hole conductor which enhanced PCE values and improved the device stability. Spiro-OMeTAD (2,2',7,7'-tetrakis(N,N'-di-p-methoxyphenylamine)- 9,9
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Benbakoura, Mansour. "Evolution des étoiles de faible masse en interaction : observations multi-techniques et modélisation des systèmes multiples." Thesis, Université de Paris (2019-....), 2019. http://www.theses.fr/2019UNIP7027.

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Cette thèse est consacrée à l'étude des étoiles de faible masse ayant dans leur environnement proche d'autres étoiles ou des planètes. Nous nous sommes concentrés sur l'influence des interactions avec ces compagnons sur l'évolution stellaire ainsi que leurs conséquences observables.Dans la première partie, nous présentons le modèle d'évolution des systèmes étoile–planète que nous avons développé au cours de cette thèse, nommé ESPEM (Évolution des Systèmes Planétaires Et Magnétisme). Ce modèle prend en compte de façon ab-initio des effets du vent stellaire magnétisé et de la dissipation de maré
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Hawkins, Keith A. "Searching for Solar-Type Hypervelocity Stars." Ohio University Honors Tutorial College / OhioLINK, 2013. http://rave.ohiolink.edu/etdc/view?acc_num=ouhonors1367583430.

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Notsu, Yuta. "Observational studies on solar-type superflare stars." Kyoto University, 2019. http://hdl.handle.net/2433/242613.

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Corporon, Patrice. "La binarité des étoiles Ae/Be de Herbig vue par l'optique adaptative et la spectroscopie : une étude du système triple TY CrA." Phd thesis, Université Joseph Fourier (Grenoble), 1998. http://tel.archives-ouvertes.fr/tel-00724469.

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Les étoiles multiples sont nombreuses, tant parmi les objets jeunes de faible masse, les étoiles T Tauri, que parmi les astres de la Séquence Principale (SP). En ce qui concerne les étoiles jeunes de masse intermédiaire, les étoiles Ae/Be de Herbig (HAeBe), le statut de la binarité est peu connu. Nous avons réalisé une recherche systématique de binaires HAeBe en utilisant deux techniques: l'imagerie à haute résolution angulaire avec la méthode de l'Optique Adaptative d'une part, et la spectroscopie visible à haute résolution d'autre part. Ces techniques complémentaires nous ont permis d'identi
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Hamilton, Devon. "Observational signatures of convection in solar type stars." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2001. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp04/NQ58914.pdf.

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Mamajek, Eric E. "Identification and characterization of young, nearby, solar-type stars." Diss., The University of Arizona, 2004. http://hdl.handle.net/10150/280625.

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Post-T Tauri stars (PTTSs) are low-mass, pre-MS stars which have ceased accreting, and are not necessarily near star-forming molecular clouds. Historically, they have been difficult to identify due to their benign spectroscopic signatures. With recent all-sky X-ray surveys and proper motion catalogs, it is now possible to find PTTSs in large numbers. The nearest PTTSs will be important targets for future imaging surveys characterizing dust disks and planetary systems around young solar analogs. The goal of this work is to systematically identify samples of PTTSs, investigate the evolution of c
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Books on the topic "Solar-type star"

1

Hamilton, Devon. Observational signatures of convection in solar type stars. Graduate Department of Astronomy and Astrophysics, University of Toronto, 2001.

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2

Rüdiger, G. Differential rotation and stellar convection: Sun and solar-type stars. Gordon and Breach Science Publishers, 1989.

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Rüdiger, Günther. Differential rotation and stellar convection: Sun and solar-type stars. Gordon and Breach Science Publishers, 1989.

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Space Telescope Science Institute (U. Survey of Chromospheric Emission and Rotation Among Solar-Type Stars in the Solar Neighborhood. s.n, 1985.

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Hotta, Hideyuki. Thermal Convection, Magnetic Field, and Differential Rotation in Solar-type Stars. Springer Japan, 2015. http://dx.doi.org/10.1007/978-4-431-55399-1.

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(Translator), Svetlana Knyazeva, ed. Solar-Type Activity in Main-Sequence Stars. Springer, 2005.

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Gershberg, Roald E. Solar-Type Activity in Main-Sequence Stars. Springer, 2008.

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Gershberg, Roald E. E., and Svetlana Knyazeva. Solar-Type Activity in Main-Sequence Stars. Springer, 2010.

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Solar-Type Activity in Main-Sequence Stars. Springer-Verlag, 2005. http://dx.doi.org/10.1007/3-540-28243-2.

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Hotta, Hideyuki. Thermal Convection, Magnetic Field, and Differential Rotation in Solar-type Stars. Springer, 2015.

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Book chapters on the topic "Solar-type star"

1

Hartquist, T. W., and R. Rosner. "Models of Solar-type Coronae." In Activity in Cool Star Envelopes. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2951-7_31.

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Tuominen, I., G. Rüdiger, and A. Brandenburg. "Observational Constraints for Solar-Type Dynamos." In Activity in Cool Star Envelopes. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2951-7_2.

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Mamajek, Eric E. "Solar-Type Post-T Tauri Stars in the Nearest OB Subgroups." In Open Issues in Local Star Formation. Springer Netherlands, 2003. http://dx.doi.org/10.1007/1-4020-2600-5_4.

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Shakhovskaya, N. I. "Some Physical Consequences from the Flare Statistics of the UV Cet Type Stars in the Solar Neighbourhood." In Flare Stars in Star Clusters, Associations and the Solar Vicinity. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0607-5_13.

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Altrock, Richard C. "Coronal-Hole Detectability on Solar-Type Stars." In Radio Stars. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5420-5_34.

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Reetz, Johannes. "Oxygen Abundances in Solar-Type Stars." In Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4213-7_27.

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Hartmann, L. "Mass Loss From Solar-Type Stars." In Progress in Solar Physics. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-4588-3_29.

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Reetz, Johannes. "Oxygen Abundance in Solar-Type Stars." In Chemical Evolution from Zero to High Redshift. Springer Berlin Heidelberg, 1999. http://dx.doi.org/10.1007/978-3-540-48360-1_14.

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Bertout, Claude, and Francois Ménard. "The Nature of Young Solar-Type Stars." In The Origin of Stars and Planetary Systems. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4509-1_10.

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Bouchy, François, and Fabien Carrier. "Present Observational Status of Solar-Type Stars." In Asteroseismology Across the HR Diagram. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-0799-2_4.

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Conference papers on the topic "Solar-type star"

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Dimitrijević, Milan S., Cristiana Dumitrache, Vasile Mioc, and Nedelia A. Popescu. "Influence of Collisions with Charged Particles on Solar Type Star Spectra; Investigations on Belgrade Astronomical Observatory." In Flows, Boundaries, Interactions. AIP, 2007. http://dx.doi.org/10.1063/1.2790350.

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Farkas, Ladislau, Vasile Mioc, Cristiana Dumitrache, and Nedelia A. Popescu. "The Beta Cephei Type Variable Star BW Vulpeculae." In EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP, 2008. http://dx.doi.org/10.1063/1.2993689.

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Michaud, George. "Particle transport in solar type stars." In AIP Conference Proceedings Vol.126. AIP, 1985. http://dx.doi.org/10.1063/1.35165.

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Honda, Satoshi, Yuta Notsu, Hiroyuki Maehara, et al. "Lithium Abundance of the Solar-Type Superflare Stars." In Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016). Journal of the Physical Society of Japan, 2017. http://dx.doi.org/10.7566/jpscp.14.020303.

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Fekel, Francis C., B. Zuckerman, Michael H. Williamson, Gregory W. Henry, M. P. Muno, and Eric Stempels. "The Dusty, Solar Type Spectroscopic Binary BD +20 307." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099246.

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Bondar’, N. I., M. M. Katsova, and M. A. Livshits. "CYCLES ON SOLAR-TYPE STARS AND MORE COOL DWARFS." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2018. http://dx.doi.org/10.31725/0552-5829-2018-67-70.

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Giampapa, Mark, William Sherry, Eric Craine, Roy Tucker, and Eric Stempels. "Photometric variability of solar-type members of the Pleiades open cluster." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099197.

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Claudi, R. U., S. Benatti, E. Carolo, A. Bonanno, and Eric Stempels. "Detection of p-modes in solar type stars with SARG@TNG." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099214.

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Chabrier, G., I. Baraffe, J. Leconte, J. Gallardo, T. Barman, and Eric Stempels. "The mass-radius relationship from solar-type stars to terrestrial planets: a review." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099078.

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Strom, Stephen E., Suzan Edwards, and Michael F. Skrutskie. "Evolutionary timescales for circumstellar disks associated with solar-type pre-main sequence stars." In Astrophysics from the Moon. AIP, 1990. http://dx.doi.org/10.1063/1.39359.

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