arXiv · astro-ph/0209298
Search for ultraluminous X-ray sources in nearby galaxies
Abstract
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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L. Foschini, G. Di Cocco, L. C. Ho, L. Bassani, M. Cappi, M. Dadina, F. Gianotti, G. Malaguti, F. Panessa, E. Piconcelli, J. B. Stephen, M. Trifoglio. 2002-09-16. Search for ultraluminous X-ray sources in nearby galaxies. https://arxiv.org/abs/astro-ph/0209298
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