A multi-model approach to X-ray pulsars
The emission characteristics of X-ray pulsars are governed by magnetospheric accretion within the Alfvén radius, leading to a direct coupling of accretion column properties and interactions at the magnetosphere. The complexity of the physical processes governing the formation of radiation within the...
Wedi'i Gadw mewn:
| Prif Awduron: | , , , , , , , , , , , , , , , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
EDP Sciences
2014-01-01
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| Cyfres: | EPJ Web of Conferences |
| Mynediad Ar-lein: | http://dx.doi.org/10.1051/epjconf/20136402003 |
| Tagiau: |
Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!
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