Results 11 to 20 of about 172,722 (314)

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

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

The origin and evolution of magnetic white dwarfs in close binary stars [PDF]

open access: yesPublished by Nature Astronomy (2021), 2021
The origin of magnetic fields in white dwarfs remains a fundamental unresolved problem in stellar astrophysics. In particular, the very different fractions of strongly (exceeding 1 MG) magnetic white dwarfs in evolutionarily linked populations of close white dwarf binary stars cannot be reproduced by any scenario suggested so far.
arxiv   +1 more source

Evidence of Stellar Oscillations in the Post-common-envelope Binary Candidate ASASSN-V J205543.90+240033.5

open access: yesThe Astrophysical Journal Letters, 2023
ASASSN-V J205543.90+240033.5 (ASJ2055) is a possible post-common-envelope binary system. Its optical photometric data show an orbital variation of about 0.52 days and a fast period modulation of P _0 ∼ 9.77 minutes, whose origin is unknown.
J. Takata   +9 more
doaj   +1 more source

Diffusion of neon in white dwarf stars [PDF]

open access: yesPhysical Review E, 2010
Sedimentation of the neutron rich isotope $^{22}$Ne may be an important source of gravitational energy during the cooling of white dwarf stars. This depends on the diffusion constant for $^{22}$Ne in strongly coupled plasma mixtures. We calculate self-diffusion constants $D_i$ from molecular dynamics simulations of carbon, oxygen, and neon mixtures. We
J. Hughto   +3 more
openaire   +4 more sources

Evaluating the effectiveness of physical exercise in improving standardized testing performances through attention indices

open access: yesBrain and Behavior, Volume 12, Issue 12, December 2022., 2022
Graphical Abstract Paired‐samples t‐tests showed that after exercise, subjects displayed increased reading speed and fewer eye drifts, coupled with increased mean scores. This study demonstrated that running, an acute, coordinative, aerobic exercise, improves attention and increases the testing performance of the SAT reading.
Jeffrey Huang   +3 more
wiley   +1 more source

Maximum mass ratio of AM CVn-type binary systems and maximum white dwarf mass in ultra-compact X-ray binaries [PDF]

open access: yesSerbian Astronomical Journal, 2011
AM CVn-type stars and ultra-compact X-ray binaries are extremely interesting semi-detached close binary systems in which the Roche lobe filling component is a white dwarf transferring mass to another white dwarf, neutron star or a black hole ...
Arbutina Bojan
doaj   +1 more source

A radio-pulsing white dwarf binary star [PDF]

open access: yesNature, 2016
White dwarfs are compact stars, similar in size to Earth but ~200,000 times more massive. Isolated white dwarfs emit most of their power from ultraviolet to near-infrared wavelengths, but when in close orbits with less dense stars, white dwarfs can strip material from their companions, and the resulting mass transfer can generate atomic line and X-ray ...
L. K. Hardy   +28 more
openaire   +11 more sources

White dwarf stars with carbon atmospheres [PDF]

open access: yesNature, 2007
White dwarfs represent the endpoint of stellar evolution for stars with initial masses between approximately 0.07 and 8-10, where is the mass of the Sun (more massive stars end their life as either black holes or neutron stars). The theory of stellar evolution predicts that the majority of white dwarfs have a core made of carbon and oxygen, which ...
Dufour, Patrick   +3 more
openaire   +5 more sources

Hot white dwarfs and pre-white dwarfs discovered with SALT [PDF]

open access: yesMNRAS 519 (2023), 2321-2330, 2023
The Southern African Large Telescope (SALT) survey of helium-rich hot subdwarfs aims to explore evolutionary pathways amongst groups of highly-evolved stars. The selection criteria mean that several hot white dwarfs and related objects have also been included. This paper reports the discovery and analysis of eight new very hot white dwarf and pre-white
arxiv   +1 more source

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