Multidimensional Nova Simulations with an Extended Buffer and Lower Initial Mixing Temperatures
A classical nova is a thermonuclear runaway initiated on a white dwarf accreting solar-like material from its stellar companion. Once the white dwarf accretes enough mass, the pressure at the base of the accreted layer reaches a critical point, leading to the ignition of the hydrogen fuel at their i...
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| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Maynooth Academic Publishing
2025-04-01
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| Series: | The Open Journal of Astrophysics |
| Online Access: | https://doi.org/10.33232/001c.136890 |
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