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XMM-Newton study of soft excess X-ray emission in clusters of galaxies

✍ Scribed by J.S. Kaastra; R. Lieu; T. Tamura; F.B.S. Paerels; J.W. den Herder

Publisher
Elsevier Science
Year
2004
Tongue
English
Weight
397 KB
Volume
34
Category
Article
ISSN
0273-1177

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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