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Cumulative luminosity functions of the X-ray point source population in M31

Published online by Cambridge University Press:  12 May 2006

L. Shaw Greening ,
C. Tonkin ,
R. Barnard ,
U. Kolb  and
J. P. Osborne
L. Shaw Greening
Affiliation:
Open University, Walton Hall, Milton Keynes, MK7 6AA, UK email: L.Shaw-Greening@open.ac.uk
C. Tonkin
Affiliation:
Open University, Walton Hall, Milton Keynes, MK7 6AA, UK email: L.Shaw-Greening@open.ac.uk
R. Barnard
Affiliation:
Open University, Walton Hall, Milton Keynes, MK7 6AA, UK email: L.Shaw-Greening@open.ac.uk
U. Kolb
Affiliation:
Open University, Walton Hall, Milton Keynes, MK7 6AA, UK email: L.Shaw-Greening@open.ac.uk
J. P. Osborne
Affiliation:
University of Leicester, University Road, Leicester, LE1 7RH, UK
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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.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S230: Populations of High Energy Sources in Galaxies , August 2005 , pp. 377 - 378
Copyright
2006 International Astronomical Union