Reference : XMM-Newton high-resolution X-ray spectroscopy of the Wolf-Rayet object WR25 (WN6ha+O4f)
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
Engineering, computing & technology : Aerospace & aeronautics engineering
http://hdl.handle.net/2268/15902
XMM-Newton high-resolution X-ray spectroscopy of the Wolf-Rayet object WR25 (WN6ha+O4f)
English
Raassen, A. J. J. [> > > >]
van der Hucht, K. A. [> > > >]
Mewe, R. [> > > >]
Antokhin, I. [> > > >]
Rauw, Grégor mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE) >]
Vreux, Jean-Marie mailto [Université de Liège - ULg > Département d'astrophysique]
Schmutz, W. [> > > >]
Gudel, M. [> > > >]
2003
Advances in Space Research
Pergamon-Elsevier Science Ltd
32
6
Connections and Reconnections in Solar and Stellar Coronae
1161-1165
Yes (verified by ORBi)
International
0273-1177
Kidlington
[en] We report the analysis of the X-ray spectrum of the Wolf-Rayet star WR 25, observed by RGS and EPIC-MOS on board XMM-Newton. Temperatures up to 40 MK have been determined. Strong absorption, exceeding the value due to the Inter Stellar Medium (ISM) has been detected and assigned to the dense stellar wind. (C) 2003 COSPAR. Published by Elsevier Ltd. All rights reserved.
http://hdl.handle.net/2268/15902

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