X-ray sources and their optical counterparts in the globular cluster M 22

被引:22
|
作者
Webb, NA
Serre, D
Gendre, B
Barret, D
Lasota, JP
Rizzi, L
机构
[1] Ctr Etud Spatiale Rayonnements, F-31028 Toulouse 04, France
[2] Inst Astrophys, F-75014 Paris, France
[3] Osserv Astron Padova, INAF, I-35122 Padua, Italy
[4] CNR, Ist Astrofis Spaziale & Fis Cosm, Rome, Italy
关键词
Galaxy : globular clusters : individual : M 22; X-rays : general; stars : binaries : general; galaxies : clusters : general;
D O I
10.1051/0004-6361:20040399
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using XMM-Newton EPIC imaging data, we have detected 50 low-luminosity X-ray sources in the field of view of M 22, where 5+/-3 of these sources are likely to be related to the cluster. Using differential optical photometry, we have identified probable counterparts to those sources belonging to the cluster. Using X-ray spectroscopic and timing studies, supported by the optical colours, we propose that the most central X-ray sources in the cluster are cataclysmic variables, millisecond pulsars, active binaries and a blue straggler. We also identify a cluster of galaxies behind this globular cluster.
引用
收藏
页码:133 / 143
页数:11
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