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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| 發表在: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , , , |
| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
Universidad Nacional Autónoma de México
2007
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| 主題: | |
| 在線閱讀: | https://www.redalyc.org/articulo.oa?id=57130002 |
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