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121
Evidence of Stellar Oscillations in the Post-common-envelope Binary Candidate ASASSN-V J205543.90+240033.5
Published 2023-01-01Subjects: Get full text
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122
Formation of PSR J1012+5307 with an Extremely Low-mass White Dwarf: Testing Magnetic Braking Models
Published 2024-01-01Subjects: Get full text
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123
White Dwarf Photospheric Abundances in Cataclysmic Variables. III. Five Dwarf Novae with an Evolved Secondary Donor Star
Published 2023-01-01Subjects: “…White dwarf stars…”
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124
XMM-Newton Detection of X-Ray Emission from the Metal-polluted White Dwarf G 29-38
Published 2023-01-01Subjects: “…White dwarf stars…”
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125
Dimming the Lights: 2D Simulations of Deflagrations of Hybrid C/O/Ne White Dwarfs Using FLASH
Published 2023-01-01Subjects: Get full text
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126
The Morphology of the Asteroidal Dust around White Dwarf Stars: Optical and Near-infrared Pulsations in G29-38
Published 2024-01-01Subjects: Get full text
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127
Stable Up-Down Quark Matter Nuggets, Quark Star Crusts, and a New Family of White Dwarfs
Published 2021-09-01Subjects: Get full text
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128
Seismic Signatures of the 12C(α, γ)16O Reaction Rate in White Dwarf Models with Overshooting
Published 2023-01-01Subjects: Get full text
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129
Atmospheric circulation of tidally locked gas giants with increasing rotation and implications for white-dwarf-brown-dwarf systems
Published 2020“…Nevertheless, there exist a class of gas-giant, highly irradiated objects—brown dwarfs orbiting white dwarfs in extremely tight orbits—whose orbital and hence rotation periods are as short as 1–2 hr. …”
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130
A Young White Dwarf Orbiting PSR J1835−3259B in the Bulge Globular Cluster NGC 6652
Published 2023-01-01Subjects: Get full text
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131
Towards precise constraints in modified gravity: bounds on alternative coupling gravity using white dwarf mass-radius measurements
Published 2023-06-01“…We propose a new idea for constraining alternative theories of gravity using temperature-dependent white dwarf (WD) mass-radius (MR) observational data. …”
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132
Seismological Studies of Pulsating DA White Dwarfs Observed with the Kepler Space Telescope and K2 Campaigns 1–8
Published 2023-01-01Subjects: “…White dwarf stars…”
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133
Constraining the White-dwarf Mass and Magnetic Field Strength of a New Intermediate Polar through X-Ray Observations
Published 2023-01-01“…We have developed a physically realistic model that considers a finite magnetosphere radius, X-ray absorption from the preshock region, and reflection from the white-dwarf (WD) surface to properly determine the IP properties, especially its WD mass. …”
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134
Spectra of V1405 Cas at the Very Beginning Indicate a Low-mass ONeMg White Dwarf Progenitor
Published 2023-01-01“…The lowest possible mass of ONeMg white dwarfs (WDs) has not been clarified despite its importance in the formation and evolution of WDs. …”
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135
Physical properties of dust particles around white dwarf in far infrared sky at 12.8o galactic latitude
Published 2018-12-01Article -
136
ELM of ELM-WD: An Extremely-low-mass Hot Star Discovered in LAMOST Survey
Published 2023-01-01Subjects: “…White dwarf stars…”
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137
Sensitivity Calibration of Far-Ultraviolet Imaging Spectrograph
Published 2004-12-01Subjects: Get full text
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138
The Optically Thick Rotating Magnetic Wind from a Massive White Dwarf Merger Product. II. Axisymmetric Magnetohydrodynamic Simulations
Published 2024-01-01Subjects: Get full text
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139
A possible critical heating from decay reaction and new upper limit of the magnetic monopole flux for the supermassive white dwarfs
Published 2024-01-01“…Abstract We present the new upper limit of the magnetic monopole (MM) flux and discuss three MM models of the heating resource for supermassive white dwarfs (WDs) by considering the effect of temperature on thermonuclear reaction and mass radius relation of WDs based on the catalytic nuclear decay by MM. …”
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140
What Powered the Kilonova-like Emission after GRB 230307A in the Framework of a Neutron Star–White Dwarf Merger?
Published 2024-01-01“…Here we propose that the origin of GRB 230307A is a neutron star–white dwarf (NS–WD) merger as this could naturally explain the long duration and the large physical offset from the center of its host galaxy. …”
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