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
openaire +2 more sources
2MASS J035523.37+113343.7: A YOUNG, DUSTY, NEARBY, ISOLATED BROWN DWARF RESEMBLING A GIANT EXOPLANET. [PDF]
Faherty JK +4 more
europepmc +1 more source
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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Globular clusters, Hipparcos, and the age of the galaxy. [PDF]
Reid N.
europepmc +1 more source
Classification of LAMOST spectra of B-type and hot subdwarf stars using kernel support vector machine. [PDF]
Tahir M +5 more
europepmc +1 more source
The Evolution of Compact Binary Star Systems. [PDF]
Postnov KA, Yungelson LR.
europepmc +1 more source
Exploring central star variability of planetary nebulae using gaia photometry. [PDF]
NegmEldin MA, Ali A, Hamed GM, Essam A.
europepmc +1 more source
Measuring cosmological parameters. [PDF]
Freedman WL.
europepmc +1 more source
Galaxies and large scale structure at high redshifts. [PDF]
Steidel CC.
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The abundances of carbon and nitrogen in the atmospheres of classical Be stars. [PDF]
Peters GJ +4 more
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