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Статті в журналах з теми "Milkyway"

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Автор: Grafiati

Опубліковано: 6 вересня 2023

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1

MAKINO, JUNICHIRO. "GRAPE AND PROJECT MILKYWAY." Journal of The Korean Astronomical Society 38, no. 2 (June 1, 2005): 165–68. http://dx.doi.org/10.5303/jkas.2005.38.2.165.

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2

Liao, Xiangke, Liquan Xiao, Canqun Yang, and Yutong Lu. "MilkyWay-2 supercomputer: system and application." Frontiers of Computer Science 8, no. 3 (May 26, 2014): 345–56. http://dx.doi.org/10.1007/s11704-014-3501-3.

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3

Ryś, S., K. T. Chyży, A. Kus, E. Pazderski, M. Soida, and M. Urbanik. "Toruń 6-cm polarimetry of the MilkyWay." Astronomische Nachrichten 327, no. 5-6 (June 2006): 493–94. http://dx.doi.org/10.1002/asna.200610568.

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4

Xu, Weixia, Yutong Lu, Qiong Li, Enqiang Zhou, Zhenlong Song, Yong Dong, Wei Zhang, et al. "Hybrid hierarchy storage system in MilkyWay-2 supercomputer." Frontiers of Computer Science 8, no. 3 (June 2014): 367–77. http://dx.doi.org/10.1007/s11704-014-3499-6.

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5

Liao, Xiangke. "MilkyWay-2: back to the world Top 1." Frontiers of Computer Science 8, no. 3 (April 8, 2014): 343–44. http://dx.doi.org/10.1007/s11704-014-4901-0.

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6

Kuperjanov, Andres. "Names in Estonian Folk Astronomy - from 'Bird's Way' to 'Milky Way'." Folklore: Electronic Journal of Folklore 22 (2002): 49–61. http://dx.doi.org/10.7592/fejf2002.22.milkyway.

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7

Chu, Yiu-Wai. "Johnnie To's “northern expedition:” from Milkyway Image toDrug War." Inter-Asia Cultural Studies 16, no. 2 (April 3, 2015): 192–205. http://dx.doi.org/10.1080/14649373.2015.1037073.

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8

Weiss, Jake, Heidi Jo Newberg, Matthew Newby, and Travis Desell. "Fitting the Density Substructure of the Stellar Halo with MilkyWay@home." Astrophysical Journal Supplement Series 238, no. 2 (September 27, 2018): 17. http://dx.doi.org/10.3847/1538-4365/aadb92.

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9

Hasto Wisnugroho, Anthonius Dhinar. "Analysis of UHT Diamond Milk Supplier Selection With Analytical Hierarchy Process (AHP) Method cafe Milkyway Coffe & Milk In Berau Regency, East Kalimantan." SAINTEKBU 14, no. 02 (April 9, 2023): 1–8. http://dx.doi.org/10.32764/saintekbu.v14i02.2741.

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Анотація:

Every business sector certainly wants consistency in production results, this can be realized through collaboration with raw material providers or suppliers who can ensure the consistent availability of raw materials because the production of raw materials is very vital. Therefore, it is necessary to have a good raw material procurement system and supplier selection so that the production process can run smoothly. Milkyway Cafe is the first pioneering UKM of beverage and food business in Berau Regency, East Kalimantan which has a special characteristic of beverage products made from milk which are liked by many customers, especially teenagers, children, and families. There are problems experienced when selecting suppliers who provide raw materials for UHT milk because there are several factors to consider, namely price, delivery, service, and accuracy of quantities. The sample of the research is the owner of the business that regulates the procurement of UHT milk. The results of the analysis and calculation of the Analytical Hierarchy Process (AHP) using Microsoft Excel stated that the chosen alternative, namely the Kompas with a weight value of 0.46, was superior to the Simpang Utama with a weighted value of 0.34 and the Tops Jaya with a weighted value of 0.20. The main factors that are prioritized in the selection of suppliers at Milkyway are service criteria with a weight value of 0.18, the accuracy of the number of goods with a weight value of 0.15, prices with a weight value of 0.08, and delivery with a weight value of 0.06.

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10

Sun, Yi. "Shaping Hong Kong cinema’s new icon: Milkyway Image at international film festivals." Transnational Cinemas 6, no. 1 (January 2, 2015): 67–83. http://dx.doi.org/10.1080/20403526.2014.1002671.

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11

Li, P. S., and H. A. Thronson. "New Particle Simulation of the Magellanic Clouds." Symposium - International Astronomical Union 190 (1999): 503–5. http://dx.doi.org/10.1017/s0074180900118716.

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We use a modified TreeSPH code to simulate the MilkyWay-LMC-SMC system using the latest observational results from Hipparcos on the proper motion of the Clouds. More than 120,000 particles are used for the simulation. Gravitational and hydrodynamic interactions among gaseous and stellar components in the system have been considered. The Magellanic Stream, some high velocity clouds, and the barred structure of LMC are reproduced. A leading gas arm from the SMC is predicted. From the simulation, the long term binary status of LMC-SMC is questioned as frequent encounters between the LMC and the SMC will have difficulty in explaining the survival of the SMC.

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12

Yin, Fukang, Guoli Wu, Jianping Wu, Jun Zhao, and Junqiang Song. "Performance Evaluation of the Fast Spherical Harmonic Transform Algorithm in the Yin–He Global Spectral Model." Monthly Weather Review 146, no. 10 (September 10, 2018): 3163–82. http://dx.doi.org/10.1175/mwr-d-18-0151.1.

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Abstract In this paper, we describe an implementation of the fast spherical harmonic transform (SHT) algorithm in the Yin–He global spectral model (YHGSM). A new analysis method is proposed to study the potential instability of interpolative decomposition and to evaluate the performance of fast SHT on the MilkyWay-2 supercomputer. The novel aspect of the proposed method is the use of the computational complexity analysis method by studying the properties of interpolative decompositions. Furthermore, three test cases are conducted to verify fast SHT in YHGSM. The results demonstrate that fast SHT is feasible and efficient for reducing the computational complexity and memory cost of SHT while still keeping enough accuracy.

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13

Bajkova, Anisa Talgatovna, and Vadim Vadimovich Bobylev. "Orbits of 152 globular clusters of the MilkyWay galaxy constructed from Gaia DR2." Research in Astronomy and Astrophysics 21, no. 7 (August 1, 2021): 173. http://dx.doi.org/10.1088/1674-4527/21/7/173.

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14

Pang, Laikwan. "Masculinity in Crisis: Films of Milkyway Image and Post-1997 Hong Kong Cinema." Feminist Media Studies 2, no. 3 (January 2002): 325–40. http://dx.doi.org/10.1080/1468077022000034826.

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15

Sun, Yi. "Renationalisation and resistance of Hong Kong cinema: Milkyway Image’s journey to Mainland China." Inter-Asia Cultural Studies 19, no. 2 (April 3, 2018): 220–33. http://dx.doi.org/10.1080/14649373.2018.1463070.

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16

Newberg, Heidi Jo, Matthew Newby, Travis Desell, Malik Magdon-Ismail, Boleslaw Szymanski, and Carlos Varela. "MilkyWay@home: Harnessing volunteer computers to constrain dark matter in the Milky Way." Proceedings of the International Astronomical Union 9, S298 (May 2013): 98–104. http://dx.doi.org/10.1017/s1743921313006273.

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AbstractMilkyWay@home is a volunteer computing project that allows people from every country in the world to volunteer their otherwise idle processors to Milky Way research. Currently, more than 25,000 people (150,000 since November 9, 2007) contribute about half a PetaFLOPS of computing power to our project. We currently run two types of applications: one application fits the spatial density profile of tidal streams using statistical photometric parallax, and the other application finds the N-body simulation parameters that produce tidal streams that best match the measured density profile of known tidal streams. The stream fitting application is well developed and is producing published results. The Sagittarius dwarf leading tidal tail has been fit, and the algorithm is currently running on the trailing tidal tail and bifurcated pieces. We will soon have a self-consistent model for the density of the smooth component of the stellar halo and the largest tidal streams. The N-body application has been implemented for fitting dwarf galaxy progenitor properties only, and is in the testing stages. We use an Earth-Mover Distance method to measure goodness-of-fit for density of stars along the tidal stream. We will add additional spatial dimensions as well as kinematic measures in a piecemeal fashion, with the eventual goal of fitting the orbit and parameters of the Milky Way potential (and thus the density distribution of dark matter) using multiple tidal streams.

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17

Barnes, Ashley, Jens Kauffmann, and Frank Bigiel. "LEGO: A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions in the Milky Way." EPJ Web of Conferences 265 (2022): 00033. http://dx.doi.org/10.1051/epjconf/202226500033.

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The current generation of high-sensitivity (sub)mm-telescopes such as the IRAM-30m and NOEMA have allowed the emission from molecular lines to become a major tool for studying the physical, kinematic and chemical properties of extragalactic systems. However, we need to develop a detailed understanding of emission lines in Milky Way molecular clouds before we can exploit extragalactic line emission data to its full potential. With this in mind, the IRAM-30m large project “Line Emission to assess Galaxy Observations” (LEGO) aims at developing a comprehensive picture of how 3mm-band emission lines in MilkyWay molecular clouds depend on a variety of environmental factors. In this proceeding, I will focus on our recent detailed investigation of the W49 massive star-forming region published in Barnes et al. 2020 [1].

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18

Newberg, Heidi Jo. "Determining distances to stars statistically from photometry." Proceedings of the International Astronomical Union 8, S289 (August 2012): 74–81. http://dx.doi.org/10.1017/s174392131202114x.

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AbstractIn determining the distances to stars within the Milky Way galaxy, one often uses photometric or spectroscopic parallaxes. In these methods, the type of each individual star is determined, and the absolute magnitude of that star type is compared with the measured apparent magnitude to determine individual distances. In this paper, we define the term statistical photometric parallax, in which statistical knowledge of the absolute magnitudes of stellar populations is used to determine the underlying density distributions of those stars. This technique has been used to determine the density distribution of the Milky Way's stellar halo and its component tidal streams, using very large samples of stars from the Sloan Digital Sky Survey. Most recently, the volunteer computing platform MilkyWay@home has been used to find the best-fitting model parameters for the density of these halo stars.

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19

Mendelsohn, Eric J., Heidi Jo Newberg, Siddhartha Shelton, Lawrence M. Widrow, Jeffery M. Thompson, and Carl J. Grillmair. "Estimate of the Mass and Radial Profile of the Orphan–Chenab Stream's Dwarf-galaxy Progenitor Using MilkyWay@home." Astrophysical Journal 926, no. 2 (February 1, 2022): 106. http://dx.doi.org/10.3847/1538-4357/ac498a.

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Abstract We fit the mass and radial profile of the Orphan–Chenab Stream’s (OCS) dwarf-galaxy progenitor by using turnoff stars in the Sloan Digital Sky Survey and the Dark Energy Camera to constrain N-body simulations of the OCS progenitor falling into the Milky Way on the 1.5 PetaFLOPS MilkyWay@home distributed supercomputer. We infer the internal structure of the OCS’s progenitor under the assumption that it was a spherically symmetric dwarf galaxy composed of a stellar system embedded in an extended dark matter halo. We optimize the evolution time, the baryonic and dark matter scale radii, and the baryonic and dark matter masses of the progenitor using a differential evolution algorithm. The likelihood score for each set of parameters is determined by comparing the simulated tidal stream to the angular distribution of OCS stars observed in the sky. We fit the total mass of the OCS’s progenitor to (2.0 ± 0.3) × 107 M ⊙ with a mass-to-light ratio of γ = 73.5 ± 10.6 and (1.1 ± 0.2) × 106 M ⊙ within 300 pc of its center. Within the progenitor’s half-light radius, we estimate a total mass of (4.0 ± 1.0) × 105 M ⊙. We also fit the current sky position of the progenitor’s remnant to be (α, δ) = ((166.0 ± 0.9)°, (−11.1 ± 2.5)°) and show that it is gravitationally unbound at the present time. The measured progenitor mass is on the low end of previous measurements and, if confirmed, lowers the mass range of ultrafaint dwarf galaxies. Our optimization assumes a fixed Milky Way potential, OCS orbit, and radial profile for the progenitor, ignoring the impact of the Large Magellanic Cloud.

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20

Bajkova, A. T., and V. V. Bobylev. "Orbits of 47 dwarf satellite galaxies of the MilkyWay in three models of the gravitational potential with different masses." Astronomical and Astrophysical Transactions, Volume 32, Numéro 3 (December 6, 2021): 177–206. http://dx.doi.org/10.17184/eac.5640.

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21

Williams, Millie S., and Terri Woods Starman. "Application of Photoperiodic Manipulation in Vegetative Specialty Floral Crop Propagation and Flowering." HortScience 33, no. 3 (June 1998): 554d—554. http://dx.doi.org/10.21273/hortsci.33.3.554d.

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Photoperiod requirements are important for optimum flower development, decreasing production time, year-round flowering, and/or for increasing vegetative growth necessary in stock plant production. The photoperiodic responses were determined for 24 vegetatively propagated specialty floral crops. Each plant species was grown at 8-, 10-, 12-, 14-, and 16-h photoperiods. Photoperiods were provided by 8 h of sunlight, then pulling black cloth and providing daylength extension with incandescent bulbs. Data collected included time to flower, flower number, and vegetative characteristics. Evolvulus nuttallianus `Blue Daze', Heliotropium arborescens `Fragrant Delight', and Orthosiphon stamineus `Lavender' were facultative short-day plants with respect to flowering. Time to flower increased as photoperiod increased. Duranta repens `Blue', Verbena hybrid `Tapien Lavender', and Verbena peruviana `Trailing Katie' were facultative long day plants with respect to flowering. Days to visible bud and first open flower decreased as photoperiod increased. Argeranthemum frutescens `Sugar Baby', Scaevola aemula `Fancy Fan Falls', and Portulaca hybrid `Apricot' had increased flower number as photoperiod increased from 8- to 16-h, although time to first flower initiation was not affected. Abutilon hybrid `Apricot', Duranta repens `Blue', Evolvulus nuttallianus `Blue Daze', Lotus berthelotii `Parrot's Beak', Lysimachia nummularia `Aurea Creeping Golden', Rhodanthe anthemoides `Milkyway', and Scaevola aemula `Fancy Fan Falls' had increased vegetative growth as photoperiod increased. All other species studied were day-neutral with regard to flowering and vegetative parameters.

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22

Soln, Josip. "Connecting dark matter particles with the primary, obscure and normal particles through implicit causality." Applied Physics Research 9, no. 3 (May 10, 2017): 1. http://dx.doi.org/10.5539/apr.v9n3p1.

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The primary, obscure and normal particles with respective limiting velocities c1, c2 and c3,solutions from bicubic equation, offer comfortable venues to tackle the newly emergent dark matter particles. Particular emphasis is given to particles with velocities of O(10-3c) ( with c the velocity of light) and whose energies are from 1eV to over 100GeV for which the congruent parameter z = 3p3mv2/2E assumes values of 10-6 and 10-7. At z = 10-6 with mc2 = 100GeV one can have E = 260GeV or with E = 1eV one can have mc2 = 0:38eV; while at z = 10-7 with mc2 = 100GeV one can have E = 2:6TeV or with E = 1eV one can have mc2 = 0:038eV. The small values of the congruent parameter z allow the limiting velocities c1, c2 and c3 as well as the resulting energy expressions be written down perturbatevly in terms of the congruent parameter z.It is shown that for mc2 = 100GeV particle in the MilkyWay Dark Matter Velocity Profile (Laha, 2016), the derived limiting velocities of primary, obscure and normal particles as dark matter particles are: c1 = 1; 7c (z = 10-7), 1:34c; 2:15c (z = 10-6); c2 = +-i1; 7c (z = 10-7), +-i1:34c; +-i2:15c (z = 10-6), and c3 = v (z = 10-7; 10-6). Perturbatively, for a very small common primary and obscure particle velocity v compared to the absolute values of their limiting velocities, one shows that the obscure particle acquires (-mv2) intrinsic negative energy with respect to the primary particle,with m being their common mass.

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23

Yi, Sun. "Building a Hong Kong Studio Brand: Milkyway’s Changing Image in Overseas Critical Reception." Canadian Journal of Film Studies 26, no. 2 (October 2017): 46–67. http://dx.doi.org/10.3138/cjfs.26.2.2017-0007.

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24

Szyłak, Jerzy. "Jaki kraj, taki Superman." Literatura i Kultura Popularna 26 (September 16, 2021): 205–15. http://dx.doi.org/10.19195/0867-7441.26.15.

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No hero similar to Superman could have appeared in communist Poland, as he represented the power of individualism and followed his own feelings of justice. Meanwhile, the communists expected one to act in a collectivity fully subordinate to the official government. This deficiency was compensated by superhero parodies. One should firstly enumerate the TV film Hydrozagadka, about a hero, who had no drawn equivalent, though he was a mockery of the comic book poetics and of the simplifications it conveys. After the communist system fell, other superhero parodies appeared, such as Ratman, Strain, Milkyman and Wilq. Also, Likwidator by Ryszard Dąbrowski constituted irreverent and mischievous comment to political events in Poland. Only later did serious superhero stories essays appear: Bler by Rafał Szłapa, Biały Orzeł by Adam Kmiołek and Jan Hardy by Jakub Kijuc. These authors take their heroes very seriously but readers can find much irony in the stories.

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25

Turner, S., and C. Jones. "The Milkybar 'Kid': Nestlé, childhood obesity and the regulation of advertising of high sugar and fat ultra-processed products." British Dental Journal 225, no. 8 (October 2018): 771–76. http://dx.doi.org/10.1038/sj.bdj.2018.868.

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26

Buzalaf, Marília Afonso Rabelo, José Mauro Granjeiro, Vanessa Eid da Silva Cardoso, Thelma Lopes da Silva, and Kelly Polido Kaneshiro Olympio. "Fluorine content of several brands of chocolate bars and chocolate cookies found in Brazil." Pesquisa Odontológica Brasileira 17, no. 3 (September 2003): 223–27. http://dx.doi.org/10.1590/s1517-74912003000300005.

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Chocolate bars and chocolate cookies are foodstuffs highly appreciated by children. The possibility of having fluorine (F) among their components, associated with an excessive consumption, may make them decisive contributors to the total daily F intake. Thus, they could participate in the establishment of dental fluorosis. The aim of this study was to analyze the fluorine concentration [F] of the chocolates bars (CB) Baton, Confeti, Garoto Ball, Kinder Ovo, M&M’s, Milkybar, Nescau, Nescau Ball, Surpresa, Surpresa Bichos, Tortuguita; and of the chocolate cookies (CC) Danyt’s, Hipopó, Nescau, Passatempo, Pokémon, Sítio do Pica-Pau Amarelo and Trakinas. Samples were purchased in Bauru, São Paulo, Brazil. Three grams of each product were previously ashed at 525°C (CB and cookies fillings) and at 550°C (cookies dough), during 4 hours. Fluorine was separated from the ash by hexamethyldisiloxane (HMDS)-facilitated diffusion. Fluorine analysis was carried out with the specific electrode. Mean [F]s ± SD and amplitude (unit mg/g) were: CB = 0.30 ± 0.45 (0.07 - 1.60, n = 12) and CC = 1.08 ± 2.64 (0.04 - 7.10, n = 7). It was concluded that some of the analyzed foods may be important contributors to the total daily F intake. As for the product that had the highest [F] (Danyt’s), when only 3 units are consumed just once a day, they may supply up to 40% of the maximum recommended daily F intake (0.07 mg/kg body weight) for a 2-year-old child (12 kg). The [F] in these products should be informed on their labels.

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27

Kovaleva, Dana, Anatoly Piskunov, Nina Kharchenko, and Ralf-Dieter Scholz. "A preliminary comparison of photometric (MWSC) and trigonometric (TGAS) distances of open cluster stars." Open Astronomy 26, no. 1 (December 20, 2017). http://dx.doi.org/10.1515/astro-2017-0427.

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AbstractThe goal of this researchwas to compare the open cluster photometric distance scale of the global survey of star clusters in the MilkyWay (MWSC) with the distances derived fromtrigonometric parallaxes fromthe Gaia DR1/TGAS catalogue and to investigate towhich degree and extent both scales agree.We compared the parallax-based and photometrybased distances of 5743 cluster stars selected as members of 1118 clusters based on their kinematic and photometric MWSC membership probabilities. We found good overall agreement between trigonometric and photometric distances of open cluster stars. The residuals between them were small and unbiased up to log(d, [pc]) ≈ 2.8. If we considered only the most populated clusters and used cluster distances obtained from the mean trigonometric parallax of their MWSC members, the good agreement of the distance scales continued up to log(d, [pc]) ≈ 3.3.

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28

Solanki, Divyesh N., Parth Bambhaniya, Dipanjan Dey, Pankaj S. Joshi, and Kamlesh N. Pathak. "Shadows and precession of orbits in rotating Janis–Newman–Winicour spacetime." European Physical Journal C 82, no. 1 (January 2022). http://dx.doi.org/10.1140/epjc/s10052-022-10045-1.

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AbstractIn this paper, we construct the rotating Janis–Newman–Winicour (JNW) naked singularity spacetime using Newman–Janis Algorithm (NJA). We analyse NJA with and without complexification methods and find that the energy conditions do satisfied when we skip the complexification step. We study the shadows cast by rotating JNW naked singularity and compare them with the shadows cast by the Kerr black hole. We find that the shadow of the rotating naked singularity can be distinguished from the shadow of the Kerr black hole. While we analyse the precession of timelike bound orbits in rotating JNW spacetime, we find that it can have a negative (or opposite) precession, which is not present in the Kerr black hole case. These novel signatures of the shadow and orbital precession in rotating JNW naked singularity spacetime could be important in the context of the recent observation of the shadow of the M87 galactic center and the stellar dynamics of ‘S-stars’ around Milkyway galactic center.

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29

Горянина, Т. "Green mass productivity and quality of winter crops as affected by cutting time." Кормопроизводство, no. 6(2019) (July 1, 2019). http://dx.doi.org/10.25685/krm.2019.2019.32189.

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Исследования проводились на полях Самарского НИИСХ, расположенных в чернозёмной степи Самарского Заволжья, с использованием сортов и линий местной селекции. В 19962005 годах в опытах изучались пять сортов озимой ржи, два сорта озимой мягкой пшеницы, четыре сорта и четыре линии тритикале. В 20162018 годах в опытах изучались два сорта озимой ржи, два сорта озимой мягкой пшеницы, четыре сорта и три линии тритикале. Цель исследований установить урожайность и качество зелёной массы тритикале в сравнении с традиционными культурами. Исходя из поставленной цели, в задачи исследований входило изучить продуктивность и качество зелёной массы тритикале, ржи и пшеницы в зависимости от сроков скашивания. Для сравнения кормовой ценности озимых культур в лаборатории технологоаналитического сервиса был проведён анализ химического состава зелёной массы растений по фазам развития. Питательность кормов характеризовалась следующими показателями: содержанием протеина, сахара, клетчатки, жира, БЭВ, каротина, кормовых единиц, а также переваримостью. За годы исследований в фазу кущения трубкования урожайность зелёной массы тритикале составила 16,85 т/га, при этом протеина в массе содержалось 18,10, сахара 14,32, клетчатки 28,90. Озимая рожь в эту фазу формирует большую урожайность зелёной массы (23,70 т/га), но качество её хуже: содержание протеина 17,70, сахара 9,94, клетчатки 29,70. Пшеница в эту фазу развития формирует меньшую урожайность (10,38 т/га), но содержит больше протеина (19,20) и меньше клетчатки (27,36). Количество протеина резко уменьшается в фазу молочновосковой спелости: на 41,4 у тритикале, на 51,4 у пшеницы и на 49,6 у ржи. Содержание сахара (11,8814,32) и жира (2,312,7) в зелёной массе тритикале остаётся практически неизменным во все изученные фазы развития. В среднем за годы исследований в тритикале содержалось 2,312,70 жира, 5,006,50 золы, 10,6018,10 протеина, 11,8814,32 сахара. По сравнению с озимой пшеницей и озимой рожью у тритикале в зелёной массе больше жира, сахара, каротина. The research was aimed to test green mass yield and quality of triticale in comparison to some conventional crops (winter rye and wheat) under different cutting times. The laboratory of Technology and Analytical Service analyzed the chemical composition of green mass cut at various growth stages. Forage nutritional value was determined on the base of protein, sugar, fiber, fat, nitrogenfree extractive, carotene, feed units as well as their digestibility. Triticale yielded 16.85 t ha1 of green mass at tilleringbooting stage, protein amounted to 18.10, sugar 14.32, fiber 28.90. Winter rye formed higher mass (23.70 t ha1), but its quality was lower: protein 17.70, sugar 9.94, fiber 29.70. Wheat was less productive (10.38 t ha1) but contained more protein (19.20) and less fiber (27.36). Protein concentration quickly dropped at milkywax stage: by 41.4 for triticale, 51.4 for wheat and by 49.6 for rye. Sugar (11.8814.32) and fat (2.312.7) stayed at the same level almost all the time in triticale green mass. Triticale had 2.312.70 of fat, 5.006.50 of ash, 10.6018.10 of protein, 11.8814.32 of sugar. Triticale exceeded winter wheat and rye in fat, sugar and carotene.

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