Models for the Circumstellar Medium of Long Gamma-Ray Burst Progenitor Candidates
We present hydrodynamical models of circumstellar medium (CSM) of long gamma-ray burst (GRB) progenitorcandidates. These are massive stars that have lost a large amount of mass in the form of stellar wind duringtheir evolution.There are two possible ways to probe the CSM of long GRB progenitors. Fir...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , , , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2007
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| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=57130002 |
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