Search for ultraluminous X-ray sources in nearby galaxies

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dc.creatorFoschini, L.
dc.creatorDi Cocco, G.
dc.creatorHo, L. C.
dc.creatorBassani, L.
dc.creatorCappi, M.
dc.creatorDadina, M.
dc.creatorGianotti, F.
dc.creatorMalaguti, G.
dc.creatorPanessa, F.
dc.creatorPiconcelli, E.
dc.creatorStephen, J. B.
dc.creatorTrifoglio, M.
dc.date2002-09-16
dc.date.accessioned2026-07-07T02:05:12Z
dc.date.available2026-07-07T02:05:12Z
dc.descriptionLittle 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.
dc.description4 pages, no figures. Presented at AGN05: Inflows, Outflows and Reprocessing around black holes, Como (Italy), 11-14 June 2002. To appear in the Proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0209298
dc.identifierhttp://arxiv.org/abs/astro-ph/0209298
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5027
dc.subjectAstrophysics
dc.titleSearch for ultraluminous X-ray sources in nearby galaxies
dc.typetext

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