Results 21 to 30 of about 4,387 (203)

Radial velocity variability and the evolution of hot subdwarf stars [PDF]

open access: yesAstronomy & Astrophysics, 2022
Hot subdwarf stars represent a late and peculiar stage in the evolution of low-mass stars, since they are likely formed by close binary interactions. In this work, we perform a radial velocity (RV) variability study of a sample of 646 hot subdwarfs with ...
S. Geier   +5 more
semanticscholar   +1 more source

A Roche Lobe-filling hot Subdwarf and White Dwarf Binary: Possible detection of an ejected common envelope? [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2022
Binaries consisting of a hot subdwarf star and an accreting white dwarf (WD) are sources of gravitational wave radiation at low frequencies and possible progenitors of type Ia supernovae if the WD mass is large enough.
Jiangdan Li   +14 more
semanticscholar   +1 more source

Discovery and analysis of three magnetic hot subdwarf stars: evidence for merger-induced magnetic fields [PDF]

open access: yes, 2022
Magnetic fields can play an important role in stellar evolution. Among white dwarfs, the most common stellar remnant, the fraction of magnetic systems is more than 20 per cent.
I. Pelisoli   +8 more
semanticscholar   +1 more source

Pulse Timing Discovery of a Three-day Companion to the Hot Subdwarf BPM 36430 [PDF]

open access: yesAstrophysical Journal, 2022
Hot subdwarf B stars are core-helium-burning objects that have undergone envelope stripping, likely by a binary companion. Using high-speed photometry from the Transiting Exoplanet Survey Satellite, we have discovered the hot subdwarf BPM 36430 is a ...
Bryce A. Smith   +4 more
semanticscholar   +1 more source

Hot Subdwarf Atmospheric Parameters, Kinematics, and Origins Based on 1587 Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR7 [PDF]

open access: yesAstrophysical Journal Supplement Series, 2021
Based on the Gaia DR2 catalog of hot subdwarf star candidates, we identified 1587 hot subdwarf stars with spectra in LAMOST DR7. We present atmospheric parameters for these stars by fitting the LAMOST spectra with Tlusty/Synspec non-LTE synthetic spectra.
Yangping Luo   +4 more
semanticscholar   +1 more source

The First Retrieval of a Substellar Subdwarf: A Cloud-free SDSS J125637.13–022452.4 [PDF]

open access: yesAstrophysical Journal, 2021
We present the first retrieval analysis of a substellar subdwarf, SDSS J125637.13−022452.4 (SDSS J1256−0224), using the Brewster retrieval code base.
Eileen C. Gonzales   +7 more
semanticscholar   +1 more source

The origin of subdwarf B stars

open access: yesBulletin de la Société royale des sciences de Liège, 2023
The origin of subdwarf B stars (sdBs) is unclear. Different formation channels are proposed including: close-binary evolution, helium-mixing on the red giant branch and the hot flasher scenario.
Callum Aubrey, R. Napiwotzki
semanticscholar   +1 more source

Kinematics of nearby Subdwarfs [PDF]

open access: yesAstrophysics and Space Science, 1999
Latex, 4 pages, 6 figures. To appear in the proceedings of the `Galaxy Evolution' conference held in Meudon, September, 21 - 25 ...
Fuchs, B., Jahreiss, H., Wielen, R.
openaire   +2 more sources

Year 1 of the ZTF high-cadence Galactic plane survey: strategy, goals, and early results on new single-mode hot subdwarf B-star pulsatos [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2021
We present the goals, strategy, and first results of the high-cadence Galactic plane survey using the Zwicky Transient Facility (ZTF). The goal of the survey is to unveil the Galactic population of short-period variable stars, including short-period ...
T. Kupfer   +20 more
semanticscholar   +1 more source

The subdwarf luminosity function [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2003
Using data from the Sloan Digital Sky Survey Early Data Release and SuperCOSMOS Sky Survey scans of POSS-I plates we identify a sample of 2600 subdwarfs using reduced proper motion methods and strict selection criteria. This forms one of the largest and most reliable samples of candidate subdwarfs known, and enables us to determine accurate luminosity ...
Digby, Andrew P.   +4 more
openaire   +2 more sources

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