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Stark Broadening and White Dwarfs [PDF]

open access: yesOpen Astronomy, 2011
White dwarf and pre-white dwarfs are the best types of stars for the application of Stark broadening research results in astrophysics, since in the atmospheres of these stars physical conditions are very favorable for this line broadening mechanism - in ...
Dimitrijević Milan S.   +3 more
doaj   +4 more sources

Asteroseismology of DAV white dwarf stars [PDF]

open access: yesOpen Astronomy, 1998
Following the recent mode identification by Clemens suggesting the hydrogen layer mass of the DAV (ZZ Ceti) stars is nearly the same, I make the extreme assumption that models with a single composition profile with a hydrogen layer mass of 1.5 × 10−4M* may be able to fit the observed pulsation periods.
Bradley P. A.
doaj   +2 more sources

White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 14 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2019
White dwarfs carry information on the structure and evolution of the Galaxy, especially through their luminosity function and initial-to-final mass relation. Very cool white dwarfs provide insight into the early ages of each population.
Kepler, So   +2 more
exaly   +4 more sources

White Dwarf.Org - Establishing a Permanent Endowment for the Whole Earth Telescope [PDF]

open access: yesOpen Astronomy, 2003
White Dwarf Research Corporation is a non-profit organization dedicated to scientific research and public education on topics relevant to white dwarf stars.
Metcalfe Travis S.
doaj   +4 more sources

Hot DAVs: a probable new class of pulsating white dwarf stars [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
We have discovered a pulsating DA white dwarf at the lower end of the temperature range 45 000–30 000 K where a few helium atmosphere white dwarfs are known. There are now three such pulsators known, suggesting that a new class of theoretically predicted
V S Dhillon   +2 more
exaly   +4 more sources

Double white dwarf mergers and elemental surface abundances in extreme helium and R Coronae Borealis stars

open access: yesMonthly Notices of the Royal Astronomical Society, 2011
The surface abundances of extreme helium (EHe) and R Coronae Borealis (RCB) stars are discussed in terms of the merger of a carbon-oxygen white dwarf with a helium white dwarf.
C Simon Jeffery, Amanda I. Karakas
exaly   +3 more sources

Diffusion of neon in white dwarf stars [PDF]

open access: yesPhysical Review E, 2010
6 pages, 5 figures, minor changes, Phys. Rev.
Horowitz, C. J.   +3 more
openaire   +3 more sources

White-Dwarf Asteroseismology With the Kepler Space Telescope

open access: yesFrontiers in Astronomy and Space Sciences, 2020
In the course of their evolution, white-dwarf stars go through at least one phase of variability in which the global pulsations they undergo allow astronomers to peer into their interiors, making it possible to shed light on their deep inner structure ...
Alejandro H. Córsico   +1 more
doaj   +1 more source

A Chondritic Solar Neighborhood

open access: yesThe Planetary Science Journal, 2023
A persistent question in exoplanet demographics is whether exoplanetary systems form from similar compositional building blocks to our own. Polluted white dwarf stars offer a unique way to address this question, as they provide measurements of the bulk ...
Isabella L. Trierweiler   +2 more
doaj   +1 more source

Catalog of Magnetic White Dwarfs with Hydrogen Dominated Atmospheres

open access: yesThe Astrophysical Journal, 2023
White dwarfs are excellent research laboratories as they reach temperatures, pressures, and magnetic fields that are unattainable on Earth. To better understand how these three physical parameters interact with each other and with other stellar features,
L. L. Amorim   +4 more
doaj   +1 more source

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