2D simulations of the double-detonation model for thermonuclear transients from low-mass carbon-oxygen white dwarfs
Date
2012
Authors
Sim, Stuart A
Fink, M
Kromer, M
Ropke, F. K.
Ruiter, A. J.
Hillebrandt, Wolfgang
Journal Title
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Volume Title
Publisher
Blackwell Publishing Ltd
Abstract
Thermonuclear explosions may arise in binary star systems in which a carbon-oxygen (CO) white dwarf (WD) accretes helium-rich material from a companion star. If the accretion rate allows a sufficiently large mass of helium to accumulate prior to ignition
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Keywords
Keywords: Binaries: close; Hydrodynamics; Methods: numerical; Radiative transfer; Supernovae: general; White dwarfs
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Source
Monthly Notices of the Royal Astronomical Society
Type
Journal article
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Restricted until
2037-12-31
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