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...
| Main Authors: | , |
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| Other Authors: | , |
| Format: | Article |
| Language: | English |
| Published: |
American Astronomical Society,
2020-12-10T22:48:17Z.
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| Subjects: | |
| Online Access: | Get fulltext |