Results 101 to 110 of about 7,790 (232)

Meet the family − the catalog of known hot subdwarf stars

open access: yesOpen Astronomy, 2017
In preparation for the upcoming all-sky data releases of the Gaia mission, we compiled a catalog of known hot subdwarf stars and candidates drawn from the literature and yet unpublished databases.
Geier Stephan   +8 more
doaj   +2 more sources

Hydrogen in hot subdwarfs formed by double helium white dwarf mergers [PDF]

open access: yes, 2016
Isolated hot subdwarfs might be formed by the merging of two helium-core white dwarfs. Before merging, helium-core white dwarfs have hydrogen-rich envelopes and some of this hydrogen may survive the merger.
Philip D. Hall, C. Jeffery
semanticscholar   +1 more source

The Arizona-Montréal Spectroscopic Survey of hot subluminous stars★

open access: yesAstronomy & Astrophysics
Context. Hot subdwarf B (sdB) and O (sdO) type stars are evolved helium-burning objects that lost their hydrogen envelope before the helium flash when their progenitors were close to the tip of the red giant branch (RGB).
Latour M.   +8 more
doaj   +1 more source

An Examination of Recent Transformations to the BV(RI)_C Photometric System from the Perspective of Stellar Models for Old Stars

open access: yes, 2010
Isochrones for ages > 4 Gyr and metallicities in the range -2.5 < [Fe/H] < +0.3 that take the diffusion of helium and recent advances in stellar physics into account are compared with observations in the Johnson-Cousins BV(RI)_C photometric system for ...
Bahcall   +51 more
core   +1 more source

MUCHFUSS - Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS [PDF]

open access: yes, 2012
The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at finding hot subdwarf stars with massive compact companions (white dwarfs with masses $M>1.0 {\rm M_{\odot}}$, neutron stars or black holes). The existence
Abazajian   +26 more
core   +2 more sources

Microscopic diffusion and subdwarfs

open access: yes, 1999
The recent distance determinations by HIPPARCOS have allowed to locate very precisely a reasonable set of subdwarfs in the HR diagram. A detailed comparison with evolutionary models is now possible and it has been recently claimed that the observed lower part of the main-sequence is cooler than the computed one.
Morel, P., Baglin, A.
openaire   +2 more sources

A Universal Transition in Atmospheric Diffusion for Hot Subdwarfs Near 18,000 K [PDF]

open access: yes, 2017
In the color–magnitude diagrams of globular clusters, when the locus of stars on the horizontal branch extends to hot temperatures, discontinuities are observed at colors corresponding to ∼12,000 and ∼18,000 K.
T. Brown   +8 more
semanticscholar   +1 more source

The Classificiation of Kepler B star Variables

open access: yes, 2012
The light curves of 252 B-star candidates in the Kepler data base are analyzed in a similar fashion to that done by Balona et al. (2011) to further characterize B star variability, increase the sample of variable B stars for future study, and to identify
Jackiewicz, Jason   +2 more
core   +1 more source

The Formation of Blue Large-amplitude Pulsators from White-dwarf Main-sequence Star Mergers

open access: yesThe Astrophysical Journal, 2023
Blue large-amplitude pulsators (BLAPs) are hot low-mass stars that show large-amplitude light variations likely due to radial oscillations driven by iron group opacities. Period changes provide evidence of both secular contraction and expansion among the
Xianfei Zhang   +3 more
doaj   +1 more source

Classification of Metal-Deficient Dwarfs in the Vilnius Photometric System

open access: yesOpen Astronomy, 2003
Methods used for the quantitative classification of metal-deficient stars in the Vilnius photometric system are reviewed. We present a new calibration of absolute magnitudes for dwarfs and subdwarfs, based on Hipparcos parallaxes.
Lazauskaitė R.   +2 more
doaj   +1 more source

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