A multi-model approach to X-ray pulsars

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 th...

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Bibliographic Details
Main Authors: Schönherr G., Schwarm F., Falkner S., Becker P., Wilms J., Dauser T., Wolff M. T., Wolfram K., West B., Pottschmidt K., Kretschmar P., Ferrigno C., Klochkov D., Nishimura O., Kreykenbohm I., Caballero I., Staubert R.
Format: Article
Language:English
Published: EDP Sciences 2014-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136402003

Internet

http://dx.doi.org/10.1051/epjconf/20136402003

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