Results 101 to 110 of about 7,790 (232)
Meet the family − the catalog of known hot subdwarf stars
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of the Gaia mission, we compiled a catalog of known hot subdwarf stars and candidates drawn from the literature and yet unpublished databases.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]
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★
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
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]
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
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]
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
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
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
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

