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
相关论文
共 50 条
  • [21] Distant cluster hunting. II. A comparison of X-ray and optical cluster detection techniques and catalogs from the ROSAT optical X-ray survey
    Donahue, M
    Scharf, CA
    Mack, J
    Lee, YP
    Postman, M
    Rosati, P
    Dickinson, M
    Voit, GM
    Stocke, JT
    ASTROPHYSICAL JOURNAL, 2002, 569 (02) : 689 - 719
  • [22] A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779
    Hopwood, MEL
    Evans, A
    Roberts, TP
    Burleigh, MR
    Odenkirchen, M
    Beardmore, AP
    O'Brien, T
    Jeffries, RD
    Penny, A
    Eyres, SPS
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2000, 316 (01) : L5 - L8
  • [23] BeppoSAX spectroscopy of the globular cluster X-ray source XB 1746-371 (NGC 6441)
    Parmar, AN
    Oosterbroek, T
    Guainazzi, M
    Segreto, A
    Dal Fiume, D
    Stella, L
    ASTRONOMY & ASTROPHYSICS, 1999, 351 (01) : 225 - 232
  • [24] A curious source of extended X-ray emission in the outskirts of globular cluster GLIMPSE-C01
    Mirabal, N.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 402 (02) : 1391 - 1396
  • [25] Influence of cluster environments on X-ray cluster morphology
    Hashimoto, Yasuhiro
    Henry, J. Patrick
    Boehringer, Hans
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2007, 380 (02) : 835 - 838
  • [26] Classifying X-ray sources in external galaxies from X-ray colors
    Prestwich, AH
    Irwin, JA
    Kilgard, RE
    Krauss, MI
    Zezas, A
    Primini, F
    Kaaret, P
    Boroson, B
    ASTROPHYSICAL JOURNAL, 2003, 595 (02) : 719 - 726
  • [27] An optical catalog of the Chandra Large Area Synoptic X-ray Survey sources
    Steffen, AT
    Barger, AJ
    Capak, P
    Cowie, LL
    Mushotzky, RF
    Yang, Y
    ASTRONOMICAL JOURNAL, 2004, 128 (04) : 1483 - 1500
  • [28] Chandra observations and optical identification of hard X-ray sources discovered with ASCA
    Watanabe, S
    Akiyama, M
    Ueda, Y
    Ohta, K
    Mushotzky, R
    Takahashi, T
    Yamada, T
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2002, 54 (05) : 683 - 694
  • [29] An anomalous low-state from the globular cluster X-ray source X 1732-304 (Terzan 1)
    Guainazzi, M
    Parmar, AN
    Oosterbroek, T
    ASTRONOMY & ASTROPHYSICS, 1999, 349 (03): : 819 - 824
  • [30] SWIFT REVEALS A ∼5.7 DAY SUPER-ORBITAL PERIOD IN THE M31 GLOBULAR CLUSTER X-RAY BINARY XB158
    Barnard, R.
    Garcia, M. R.
    Murray, S. S.
    ASTROPHYSICAL JOURNAL, 2015, 801 (01)