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Direct imaging searches for planets around white dwarf stars
Published 2005“…We discuss current searches for planetary companions to white dwarfs, including our own "DODO" programme. At the time of writing, no planetary companion to a white dwarf has been detected. …”
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Compact objects in astrophysics : white dwarfs, neutron stars, and black holes /
Published 2007Subjects: Get full text
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Measuring the Mass–Radius Relation of White Dwarfs Using Wide Binaries
Published 2024-01-01Subjects: “…White dwarf stars…”
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Effects of modified gravity on microscopic properties and cooling timescale of white dwarfs
Published 2024-03-01Subjects: Get full text
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Stark Broadening of Cr III Spectral Lines: DO White Dwarfs
Published 2018-04-01Subjects: Get full text
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Halted-pendulum Relaxation: Application to White Dwarf Binary Initial Data
Published 2023-01-01Subjects: Get full text
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New Chondritic Bodies Identified in Eight Oxygen-bearing White Dwarfs
Published 2023-01-01Subjects: Get full text
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GRB 211211A: A Neutron Star–White Dwarf Merger?
Published 2023-01-01Subjects: Get full text
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White Dwarfs with Infrared Excess from LAMOST Data Release 5
Published 2023-01-01Subjects: “…White dwarf stars…”
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The runaway velocity of the white dwarf companion in the double detonation scenario of supernovae
Published 2024-01-01Get full text
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An Extremely Massive White Dwarf Escaped from the Hyades Star Cluster
Published 2023-01-01Subjects: “…White dwarf stars…”
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Imprint of the Crystallization of Binary White Dwarfs on Gravitational Wave Observations with LISA
Published 2023-02-01Subjects: “…white dwarf…”
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Effects of Spiralling Trajectories on White Dwarf Spectra: High Rydberg States
Published 2023-11-01“…It has been recently suggested that white dwarf diagnostics could be in error and should be revised because of the effect of the magnetic field on spiralling trajectories of the plasma particles (mainly electrons), predicting a dramatic width increase for high densities of Balmer-<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>β</mi></semantics></math></inline-formula> and especially for the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>δ</mi></semantics></math></inline-formula> and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>ϵ</mi></semantics></math></inline-formula> lines. …”
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Tidal Stripping of a White Dwarf by an Intermediate-mass Black Hole
Published 2023-01-01“…During the inspiralling of a white dwarf (WD) into an intermediate-mass black hole (∼10 ^2−5 M _⊙ ), both gravitational waves (GWs) and electromagnetic (EM) radiation are emitted. …”
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EVOLUTION OF CATACLYSMIC VARIABLES AND RELATED BINARIES CONTAINING A WHITE DWARF
Published 2017“…We present a binary evolution study of cataclysmic variables (CVs) and related systems with white dwarf (WD) accretors, including for example, AM CVn systems, classical novae, supersoft X-ray sources (SXSs), and systems with giant donor stars. …”
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Accretion of a Terrestrial-Like Minor Planet by a White Dwarf
Published 2013“…We present optical and infrared characterization of the polluted DAZ white dwarf GALEX J193156.8+011745. Imaging and spectroscopy from the ultraviolet to the thermal infrared indicate that this white dwarf hosts excess infrared emission consistent with the presence of an orbiting dusty debris disk. …”
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The violent white dwarf merger scenario for the progenitors of Type Ia supernovae
Published 2016“…Recent observations suggest that some Type Ia supernovae (SNe Ia) originate from the merging of two carbon-oxygen white dwarfs (CO WDs). Meanwhile, recent hydrodynamical simulations have indicated that the accretion-induced collapse may be avoided under certain conditions when double WDs merge violently. …”
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Remnant evolution after a carbon-oxygen white dwarf merger
Published 2007“…We systematically explore the evolution of the merger of two carbon-oxygen (CO) white dwarfs. The dynamical evolution of a 0.9 Msun + 0.6 Msun CO white dwarf merger is followed by a three-dimensional SPH simulation. …”
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