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...
Furkejuvvon:
| Publikašuvnnas: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Váldodahkkit: | , , , |
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
Universidad Nacional Autónoma de México
2007
|
| Fáttát: | |
| Liŋkkat: | https://www.redalyc.org/articulo.oa?id=57130002 |
| Fáddágilkorat: |
Eai fáddágilkorat, Lasit vuosttaš fáddágilkora!
|