New XMM-newton analysis of three bright X-ray sources in M31 globular clusters, including a new black hole candidate

Astrophysical Journal

Volumn 689, Issue 2, 2008, Pages 1215-1221

  Barnard, R ^a   Stiele, H ^b   Hatzidimitriou, D ^c,d   Kong, A K H ^e   Williams, B F ^f   Pietsch, W ^b   Kolb, U C ^a   Haberl, F ^b   Sala, G ^b  

^a OPEN UNIVERSITY   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c UNIVERSITY OF CRETE   (Greece)

^d INSTITUTE OF COMPUTER SCIENCE   (Greece)

^e NATIONAL TSING HUA UNIVERSITY   (Taiwan)

^f UNIVERSITY OF WASHINGTON   (United States)

Author keywords

Galaxies: individual (M31); Methods: data analysis; X rays: binaries

Indexed keywords

EID: 58149123640     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/592594     Document Type: Article

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