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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dc.creatorFoschini, L.
dc.creatorDi Cocco, G.
dc.creatorDadina, M.
dc.creatorBassani, L.
dc.creatorCappi, M.
dc.creatorStephen, J. B.
dc.creatorTrifoglio, M.
dc.creatorGianotti, F.
dc.creatorHo, L. C.
dc.creatorMulchaey, J.
dc.creatorPanessa, F.
dc.creatorPiconcelli, E.
dc.date2002-02-13
dc.date.accessioned2026-07-07T02:02:47Z
dc.date.available2026-07-07T02:02:47Z
dc.descriptionWe 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.
dc.description4 pages, 6 figures. Proceedings Symposium "New Visions of the Universe in the XMM-Newton and Chandra era" (ESA SP-488, Ed. F. Jansen). To be published
dc.identifierhttps://arxiv.org/abs/astro-ph/0202247
dc.identifierhttp://arxiv.org/abs/astro-ph/0202247
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4166
dc.subjectAstrophysics
dc.titleFirst 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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