Observation with XMM-Newton of the globular cluster M22

Details Observation with XMM-Newton of the globular cluster M22 Observation with XMM-Newton of the globular cluster M22

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..279g&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

Scientific paper

We present preliminary results from XMM-Newton/EPIC observations of the nearby globular cluster M22. We have detected 34 low luminosity sources (< 1034.5 erg s-1) in the direction of the cluster, searching down to a luminosity of ≅ 3.0 times 1030 erg s-1. Only seven of these sources have been previously detected by either ROSAT or EINSTEIN. Three sources (two previously undetected) lie within the core radius of the cluster. For the strongest source in the observation we have a spectrum and a light curve. Finally we discuss the nature of this dim X-ray source, in light of these observations.

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