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Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9

✍ Scribed by F. Bocchino

Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
178 KB
Volume
35
Category
Article
ISSN
0273-1177

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πŸ“œ SIMILAR VOLUMES

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## Abstract The transient system SAX J1711.6–3808 was observed by XMM‐Newton during its 2001 outburst, when the source was close to its maximum outburst luminosity. Our observations show that the broad Fe emission line detected in this outburst by In' t Zand et al. (2002) has indeed a relativistic