Long term BeppoSAX-WFC monitoring of GRS 1758-258

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dc.creatorCocchi, M.
dc.creatorSmith, M. J. S.
dc.creatorMuller, J. M.
dc.creatorBazzano, A.
dc.creatorNatalucci, L.
dc.creatorUbertini, P.
dc.creatorHeise, J.
dc.creatorZand, J. J. M. in 't
dc.date1999-01-18
dc.date.accessioned2026-07-07T02:30:02Z
dc.date.available2026-07-07T02:30:02Z
dc.descriptionFollowing a series of deep observations of the Galactic Bulge region performed with the Wide Field Cameras on board BeppoSAX, it has been possible to study throughout a long time period a number of persistent X-ray sources. We report on the behaviour of GRS 1758-258, an X-ray binary suggested as a black hole candidate on the basis of its timing and spectral characteristics. The source has been monitored for almost 2 years since August 1996; preliminary results of the data analysis are shown hereafter.
dc.description4 pages, 3 figures, proc. 3rd INTEGRAL Workshop - Taormina 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9901233
dc.identifierhttp://arxiv.org/abs/astro-ph/9901233
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13699
dc.subjectAstrophysics
dc.titleLong term BeppoSAX-WFC monitoring of GRS 1758-258
dc.typetext

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