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MODERN STELLAR ASTRONOMY – 2022
We provide an analytic review of problems of the modern stellar astronomy. It mostly based on talks presented at the twelfth annual conference on Modern Stellar Astronomy, held in Caucasian Mountain Observatory of Sternberg Astronomical Institute (Kislovodsk, Russia) in November 2022.
O. Yu. Malkov +2 more
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We provide an analytic review of problems of the modern stellar astronomy. It mostly based on talks presented at the thirteenth annual conference on Modern Stellar Astronomy, held in Volgograd State University (Russia) in May 2023. The key topics for the review are Stars, Stellar Clusters and Associations, Interstellar Medium and Star Formation, Galaxy
O. Yu. Malkov +2 more
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Positional Astronomy and Stellar Masses [PDF]
In this paper are surveyed the combinations of data needed for mass determinations, the impact of radial-velocity and speckle observations, the 1983 catalog of visual-binary orbits, the current material for main-sequence and red-dwarf masses and the controversial methods and results on low mass objects.
W. D. Heintz
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X-ray astronomy of stellar coronae [PDF]
X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally attributed to the presence of a magnetic corona that contains plasma at temperatures exceeding 1 million K. Coronae are ubiquitous among these stars, yet many fundamental mechanisms operating in their magnetic fields still elude an interpretation through a ...
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Invertible Neural Networks in Astrophysics [PDF]
Modern machine learning techniques have become indispensable in many fields of astronomy and astrophysics. Here we introduce a specific class of methods, invertible neural networks, and discuss two specific applications, the prediction of stellar ...
Klessen Ralf S.
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The results of observations of selected stars orbiting the central body of our Galaxy, which, according to the latest data, has a mass of about 4 million of solar mass, are considered.
Shakht Natalia A. +2 more
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In this paper, we report on the follow-up of six potential exoplanets detected with Gaia astrometry and provide an overview of what is currently known about the nature of the entire Gaia astrometric exoplanet candidate sample, 72 systems in total.
Marcus L. Marcussen, Simon H. Albrecht
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We present a multiwavelength study of stellar flares on primarily G-type stars using overlapping time domain surveys in the near-ultraviolet (NUV) and optical regimes. The NUV (the Galaxy Evolution Explorer; GALEX) and optical (Kepler) wavelength domains
C. E. Brasseur +3 more
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