HYPERCRITICAL ACCRETION ONTO A MAGNETIZED NEUTRON STAR SURFACE: A NUMERICAL APPROACH
The properties of a new-born neutron star, produced in a core-collapse supernova, can be strongly affected by the possible late fallback which occurs several hours after the explosion. This accretion occurs in the regime dominated by neutrino cooling, explored initially in this context by Chevalier...
Wedi'i Gadw mewn:
| Cyhoeddwyd yn: | Revista Mexicana de Astronomía y Astrofísica |
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| Prif Awduron: | , , |
| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
Universidad Nacional Autónoma de México
2010
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| Pynciau: | |
| Mynediad Ar-lein: | https://www.redalyc.org/articulo.oa?id=57115522009 |
| Tagiau: |
Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!
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