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201
The Origin and Evolution of the Normal Type Ia SN 2018aoz with Infant-phase Reddening and Excess Emission
Published 2023-01-01Subjects: Get full text
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202
The Progenitors of Superluminous Type Ia Supernovae
Published 2023-01-01Subjects: Get full text
Article -
203
The Early Light Curve of the Type Ia Supernova 2021hpr in NGC 3147: Progenitor Constraints with the Companion Interaction Model
Published 2023-01-01Subjects: Get full text
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204
The Binary and the Disk: The Beauty is Found within NGC3132 with JWST
Published 2023-01-01Subjects: Get full text
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205
Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters
Published 2024-01-01Subjects: Get full text
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206
Prospects for Detecting Fast Radio Bursts in the Globular Clusters of Nearby Galaxies
Published 2023-01-01Subjects: Get full text
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207
WOCS 4540: Detailed Analysis of a very Long Orbital Period Blue Straggler
Published 2023-01-01Subjects: Get full text
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208
Precise Age for the Binary Star System 12 Com in the Coma Berenices Cluster
Published 2023-01-01Subjects: Get full text
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209
Nucleus-Acoustic Solitary Waves in Warm Degenerate Magneto-Rotating Quantum Plasmas
Published 2022-09-01Subjects: Get full text
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210
Compact objects in close orbits as gravitational wave sources: Formation scenarios and properties
Published 2024-04-01Subjects: Get full text
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211
Does Nature Allow the Formation of Ultra-compact Black Hole X-Ray Binaries via the Accretion-induced Collapse of Neutron Stars?
Published 2023-01-01Subjects: Get full text
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212
Giant Planet Engulfment by Evolved Giant Stars: Light Curves, Asteroseismology, and Survivability
Published 2023-01-01Subjects: Get full text
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213
Stark Broadening of Co II Lines in Stellar Atmospheres
Published 2020-08-01Subjects: Get full text
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214
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217
Recurrent novae: Type Ia supernovae in the making
Published 2001“…The mass of the white dwarf ranges from 1.35-1.37 M. for seven recurrent novae except for T Pyx which has a less massive white dwarf of 1.2 M.. …”
Conference item -
218
Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe.
Published 2011“…There are two classes of models: double-degenerate (involving two white dwarfs in a close binary system) and single-degenerate models. …”
Journal article -
219
Laboratory analogue of a supersonic accretion column in a binary star system.
Published 2016“…For magnetic cataclysmic variable stars, material from a late, main sequence star is pulled onto a highly magnetized (B>10 MG) white dwarf. The magnetic field is sufficiently large to direct the flow as an accretion column onto the poles of the white dwarf, a star subclass known as AM Herculis. …”
Journal article -
220
Laboratory analogue of a supersonic accretion column in a binary star system.
Published 2016“…For magnetic cataclysmic variable stars, material from a late, main sequence star is pulled onto a highly magnetized (B>10 MG) white dwarf. The magnetic field is sufficiently large to direct the flow as an accretion column onto the poles of the white dwarf, a star subclass known as AM Herculis. …”
Journal article