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2D simulations of the double-detonation model for thermonuclear transients from low-mass carbon-oxygen white dwarfs

Sim, Stuart A; Fink, M; Kromer, M; Ropke, F. K.; Ruiter, A. J.; Hillebrandt, Wolfgang

Description

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

CollectionsANU Research Publications
Date published: 2012
Type: Journal article
URI: http://hdl.handle.net/1885/67577
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1111/j.1365-2966.2011.20162.x

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