Super-Eddington Winds from Type I X-Ray Bursts
We present hydrodynamic simulations of spherically symmetric super-Eddington winds from radius-expansion type I X-ray bursts. Previous studies assumed a steady-state wind and treated the mass-loss rate as a free parameter. Using MESA, we follow the multi-zone time-dependent burning, the convective a...
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| Format: | Article |
| Language: | English |
| Published: |
American Astronomical Society
2020
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| Online Access: | https://hdl.handle.net/1721.1/128788 |