Search for relativistic beaming in ultraluminous X-ray sources

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dc.creatorFoschini, L.
dc.creatorMalaguti, G.
dc.creatorDi Cocco, G.
dc.creatorCappi, M.
dc.creatorDadina, M.
dc.creatorHo, L. C.
dc.date2003-02-07
dc.date2003-02-10
dc.date.accessioned2026-07-07T02:07:31Z
dc.date.available2026-07-07T02:07:31Z
dc.descriptionThe nature of the ultraluminous X-ray sources (ULX) is still to be understood. Several hypotheses have been suggested to explain the high X-ray luminosity: stellar mass black holes with emission collimated by relativistic effects or anisotropies in the accretion disk, intermediate mass black holes, young supernovae remnants, background active galactic nuclei. To discriminate among the above hypotheses, the search for relativistic effects can be a valuable "pathfinder". Here we propose a list of ULX candidates suitable to show relativistic beaming
dc.description5 pages, no figure. For the Proceedings of the 15th SIGRAV Conference on General Relativity and Gravitation. Corrected for a misspelled reference
dc.identifierhttps://arxiv.org/abs/astro-ph/0302143
dc.identifierhttp://arxiv.org/abs/astro-ph/0302143
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5722
dc.subjectAstrophysics
dc.titleSearch for relativistic beaming in ultraluminous X-ray sources
dc.typetext

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