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First Results from a XMM-Newton Survey of a Distance-Limited (D < 22 Mpc) Sample of Seyfert Galaxies. II - The Galactic Serendipitous Sources

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arxiv astro-ph/0202247 v1 pith:2XRTJBTK submitted 2002-02-13 astro-ph

L. Foschini , G. Di Cocco , M. Dadina , L. Bassani , M. Cappi , J. B. Stephen , M. Trifoglio , F. Gianotti
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L. C. Ho J. Mulchaey F. Panessa E. Piconcelli
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classification astro-ph
keywords galaxiesresultsxmm-newtongalacticsampleserendipitousseyfertsources
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We present preliminary results from a study with XMM-Newton of the galactic serendipitous sources in a sample of 28 nearby Seyfert galaxies (with D < 22 Mpc). We concentrate here on a subset of four galaxies, namely: NGC3185, NGC3486, NGC3941, and NGC4565. In these galaxies we found six ultraluminous X-ray source (ULX). The large collecting area of XMM-Newton makes the statistics sufficient to perform spectral fitting with simple models. We shortly discuss the results obtained so far.

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