The MHD collapsar model for GRBs: an Inflow produces an outflow
We present our recent results from numerical simulations of a magnetized ow in the vicinity of a black holein the context of the collapsar model for GRBs. The simulations show that after an initial transient, the flow settles into a complex convolution of several distinct, time-dependent flow compon...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Hovedforfatter: | |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2007
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| Online adgang: | https://www.redalyc.org/articulo.oa?id=57102707 |
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