Results 71 to 80 of about 154,154 (200)
Hubble Space Telescope Observations of UV Oscillations in WZ Sagittae During the Decline from Outburst [PDF]
We present a time series analysis of Hubble Space Telescope observations of WZ Sge obtained in 2001 September, October, November and December as WZ Sge declined from its 2001 July superoutburst.
Boris T. Gänsicke +21 more
core +2 more sources
A White Dwarf Catalog from LAMOST DR11 Using Deep Learning
White dwarfs, also referred to as degenerate dwarfs, represent the ultimate fate for the majority of stars in the Universe, unless their mass is large enough for them to evolve into black holes or neutron stars.
Shengwen Zhang, Yanxia Zhang, Chao Liu
doaj +1 more source
A Gravitational-wave-detectable Candidate Type Ia Supernova Progenitor
Type Ia supernovae (SNe Ia), critical for studying cosmic expansion, arise from thermonuclear explosions of white dwarfs, but their precise progenitor pathways remain unclear.
Emma T. Chickles +39 more
doaj +1 more source
Revisiting the Impact of Axions in the Cooling of White Dwarfs
It has been shown that the shape of the luminosity function of white dwarfs can be a powerful tool to check for the possible existence of DFSZ-axions. In particular, Isern et al.
Althaus, Leandro +2 more
core
Evolved solar systems in Praesepe [PDF]
"Copyright 2011 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics." Original paper can be found at: http://scitation.aip.org ...
Burleigh, Matt R. +3 more
core +2 more sources
Low Frequency Gravitational Waves from White Dwarf MACHO Binaries [PDF]
The possibility that Galactic halo MACHOs are white dwarfs has recently attracted much attention. Using the known properties of white dwarf binaries in the Galactic disk as a model, we estimate the possible contribution of halo white dwarf binaries to ...
Ben Kulick +4 more
core +2 more sources
Violent mergers revisited: The origin of the fastest stars in the Galaxy
Binary systems of two carbon-oxygen white dwarfs are one of the most promising candidates for the progenitor systems of Type Ia supernovae. Violent mergers, where the primary white dwarf ignites when the secondary white dwarf smashes into it while being ...
Pakmor Rüdiger +14 more
doaj +1 more source
Models for the soft X-ray emission of post-outburst classical novae
A hydrostatic and stationary white dwarf envelope model has been developed for the study of the post-outburst phases of classical novae and their soft X-ray emission.
Hernanz, Margarita, Sala, Gloria
core +1 more source
Weighing The Options: The Unseen Companion in LAMOST J2354 is Likely a Massive White Dwarf
LAMOST J235456.73+335625 (J2354) is a binary system hosting a $\sim 0.7~\rm M_\odot$ K dwarf and a $\sim 1.4~\rm M_\odot$ dark companion, supposedly a neutron star, in a 0.48d orbit.
Michael A Tucker +3 more
doaj +1 more source
A helium-burning white dwarf binary as a supersoft X-ray source. [PDF]
Greiner J +14 more
europepmc +1 more source

