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Search for ultraluminous X-ray sources in nearby galaxies

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arxiv astro-ph/0209298 v1 pith:YGRAEGZO submitted 2002-09-16 astro-ph

L. Foschini , G. Di Cocco , L. C. Ho , L. Bassani , M. Cappi , M. Dadina , F. Gianotti , G. Malaguti
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F. Panessa E. Piconcelli J.B. Stephen M. Trifoglio
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classification astro-ph
keywords sourcesultraluminousx-raybackgroundbeencurrentdifferentexplain
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Little is presently known about the nature of ultraluminous X-ray sources (ULX). Different hypotheses have been proposed to explain their properties: intermediate-mass BHs, Kerr BHs, young SNR, or background AGN. Some of the current problems and open questions in this research field are here reviewed.

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