posted on 2012-10-24, 09:08authored byL. S. Greening, C. Tonkin, R. Barnard, U. Kolb, J. P. Osborne
We present preliminary results from a detailed analysis of the X-ray point sources in
the XMM-Newton survey of M31 (e.g. Barnard et al. 2005; Pietsch et al. 2005). These
sources are expected to be mostly X-ray binaries.
History
Citation
Proceedings of the International Astronomical Union, 2005, 1, pp. 377-378
Published in
Proceedings of the International Astronomical Union
Publisher
Cambridge University Press (CUP) for International Astronomical Union (IAU)