Broad relativistic iron emission line observed in SAX J1808.4-3658
During the 2008 September-October outburst of the accreting millisecond pulsar SAX J1808.4-3658, the source was observed by both Suzaku and XMM-Newton approximately 1 day apart. Spectral analysis reveals a broad relativistic Fe K? emission line which is present in both data sets, as has recently bee...
| Main Authors: | , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
2009.
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| Subjects: | |
| Online Access: | Get fulltext |