Results 1 to 10 of about 84,708 (345)

Pulsating white dwarfs [PDF]

open access: yesEPJ Web of Conferences, 2017
The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor of five and consequently the number of known pulsating white dwarfs also by a factor of five.
Kepler S.O., Romero Alejandra D.
doaj   +3 more sources

Polluted white dwarfs reveal exotic mantle rock types on exoplanets in our solar neighborhood [PDF]

open access: yesNature Communications, 2021
While some exoplanets that once orbited Polluted white dwarfs are similar to Earth, most appear to have rock types that are exotic to our Solar System. We thus develop a new classification scheme to describe these new and novel lithologies that appear to
Keith D. Putirka, Siyi Xu
doaj   +2 more sources

The 100 pc White Dwarf Sample in the SDSS Footprint. II. A New Look at the Spectral Evolution of White Dwarfs

open access: goldThe Astrophysical Journal
We increase the spectroscopic completeness of the 100 pc white dwarf sample in the Sloan Digital Sky Survey footprint with 840 additional spectra. Our spectroscopy is 86% complete for white dwarfs hotter than T _eff  = 5000 K, where H α remains visible ...
Mukremin Kilic   +7 more
doaj   +2 more sources

MAGNETISM OF WHITE DWARFS (intermediate results of a survey for kilogauss magnetic fields in white dwarfs)

open access: greenOdessa Astronomical Publications, 2017
We shortly present intermidiate results of a survey for weak magnetic fields among degenerate stars (white dwarfs and hot subdwarf stars). Kilogauss upper limits of longitudinal magnetic fields are presented for several brightest DA white dwarfs and new ...
G. Valyavin   +6 more
doaj   +2 more sources

Ultra-low-mass and small-radius white dwarfs made of heavy elements

open access: yesFrontiers in Astronomy and Space Sciences, 2023
Seven possible ultra-low-mass and small-radius white dwarfs have been recently identified, with masses ranging from ∼0.02 M⊙ to ∼0.08 M⊙ and radii ranging from ∼ 4,270 km to 10670 km.
Cheng-Jun Xia   +8 more
doaj   +1 more source

Accreting white dwarf [PDF]

open access: yesProceedings of Supernovae: lights in the darkness — PoS(SUPERNOVA), 2008
Thermonuclear (type Ia) supernovae are explosions in accreting white dwarfs, but the exact scenario leading to these explosions is still unclear. An important step to clarify this point is to understand the behaviour of accreting white dwarfs in close binary systems.
Hernanz, Margarita, José, Jordi
openaire   +3 more sources

White-dwarf–white-dwarf galactic background in the LISA data [PDF]

open access: yesPhysical Review D, 2005
36 pages, 15 ...
Edlund, J.   +3 more
openaire   +5 more sources

Magnetism in white Dwarfs [PDF]

open access: yesSymposium - International Astronomical Union, 1971
Searches have been made for the normal and quadratic Zeeman effect and broad-band circular polarization in white dwarf stars. A positive effect has been found in Grw + 70°8247 whose continuum shows both linear and circular polarization.
J. D. Landstreet, J. R. P. Angel
openaire   +1 more source

Explosion of White Dwarfs [PDF]

open access: yesInternational Astronomical Union Colloquium, 1987
AbstractWe present models for Type I supernova light curves based on the explosion of partially solid white dwarfs in close binary systems. Studies of such explosions show that they leave bound remnants of different size. Our results reproduce quite well the maximun luminosities, the expansion velocities and the shape of the light curve.
R. Lopez, J. Isern, J. Labay, R. Canal
openaire   +1 more source

White Dwarf and Pre-White Dwarf Pulsations [PDF]

open access: yesAIP Conference Proceedings, 2009
In this review I describe the basic properties of white dwarfs and their pulsations. I then discuss some of the areas in which the pulsations can provide meaningful results, such as internal chemical profiles, possible emission of “exotic” particles, planet detection, crystallization, convection, accretion, and cosmochronology.
M. H. Montgomery   +2 more
openaire   +2 more sources

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