Results 41 to 50 of about 91 (85)

A comprehensive search for hot subdwarf stars using Gaia and TESS I. Pulsating hot subdwarf B stars

open access: yes
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
openaire   +2 more sources

Subdwarf B Stars: Tracers Of Binary Evolution

open access: yes, 2007
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
openaire   +1 more source

The Evolution of Compact Binary Star Systems. [PDF]

open access: yesLiving Rev Relativ, 2006
Postnov KA, Yungelson LR.
europepmc   +1 more source

Measuring cosmological parameters. [PDF]

open access: yesProc Natl Acad Sci U S A, 1998
Freedman WL.
europepmc   +1 more source

The abundances of carbon and nitrogen in the atmospheres of classical Be stars. [PDF]

open access: yesAstrophys Space Sci
Peters GJ   +4 more
europepmc   +1 more source

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