2D simulations of the double-detonation model for thermonuclear transients from low-mass carbon-oxygen white dwarfs
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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
| Collections | ANU 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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| File | Description | Size | Format | Image |
|---|---|---|---|---|
| 01_Sim_2D_simulations_of_the_2012.pdf | 1.44 MB | Adobe PDF | Request a copy |
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