Results 71 to 80 of about 130 (117)
Iron and nickel diffusion in subdwarf B stars
6 pages, 5 figures, to appear in ASP Conference Series, the 61st Fujihara Seminar: Progress in solar/stellar physics with helio- and ...
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A comprehensive search for hot subdwarf stars using Gaia and TESS
Hot subdwarf B (sdB) stars are evolved, subluminous, helium-burning stars that most likely form when red giant stars loose their hydrogen envelope via interactions with close companions. They play an important role in our understanding of binary evolution, stellar atmospheres, and interiors.
Murat Uzundag +7 more
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Detection of the Progenitors of Be X-ray Binaries. [PDF]
Gies D, Wang L, Peters G.
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A Kinematically Cold Structure of Candidate Young OB Stars toward the Anticenter. [PDF]
Casetti-Dinescu DI, Girard TM.
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Metal abundances in hot white dwarfs with signatures of a superionized wind. [PDF]
Werner K, Rauch T, Kruk JW.
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Subdwarf B Stars: Tracers Of Binary Evolution
Subdwarf B stars are a superb stellar population to study binary evolution. In 2001, Maxted et al. (MNRAS, 326, 1391) found that 21 out of the 36 subdwarf B stars they studied were in short period binaries. These observations inspired new theoretical work that suggests that up to 90 per cent of subdwarf B stars are in binary systems with the remaining ...
Morales-Rueda, L. +2 more
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A comprehensive search for hot subdwarf stars using Gaia and TESS I. Pulsating hot subdwarf B stars
Hot subdwarf B (sdB) stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant stars lose their hydrogen envelope via interactions with close companions. They play an important role in our understanding of binary evolution, stellar atmospheres, and interiors.
Uzundag, Murat +6 more
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Citation-based clustering of publications using CitNetExplorer and VOSviewer. [PDF]
van Eck NJ, Waltman L.
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Post-main-sequence planetary system evolution. [PDF]
Veras D.
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The Evolution of Compact Binary Star Systems. [PDF]
Postnov KA, Yungelson LR.
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