INTEGRAL monitoring of the Black Hole candidate 1E 1740.7-2942

dc.creatorDel Santo, M.
dc.creatorBazzano, A.
dc.creatorSmith, D. M.
dc.creatorBassani, L.
dc.creatorBird, A. J.
dc.creatorBouchet, L.
dc.creatorCadolle-Bel, M.
dc.creatorCapitanio, F.
dc.creatorDe Cesare, G.
dc.creatorFalanga, M.
dc.creatorFrontera, F.
dc.creatorGoldoni, P.
dc.creatorGoldwurm, A.
dc.creatorHuovelin, J.
dc.creatorKuulkers, E.
dc.creatorLund, N.
dc.creatorMalaguti, G.
dc.creatorMalizia, A.
dc.creatorMirabel, I. F.
dc.creatorNatalucci, L.
dc.creatorPaizis, A.
dc.creatorPaul, J.
dc.creatorReglero, V.
dc.creatorUbertini, P.
dc.creatorVilhu, O.
dc.creatorWinkler, C.
dc.creatorZdziarski, A.
dc.date2004-06-17
dc.date.accessioned2026-07-07T02:13:34Z
dc.date.available2026-07-07T02:13:34Z
dc.descriptionThe brightest persistent Galactic black hole candidate close to the Galactic Centre, 1E 1740.7-2942, has long been observed with INTEGRAL. In this paper, we report on the long-term hard X-ray monitoring obtained during the first year of observations as part of the Galactic Centre Deep Exposure. We discuss the temporal and spectral behaviours in different energy bands up to 250 keV, as well as the hardness-flux correlations.
dc.description6 pages, 17 figures. Proceedings of the 5th INTEGRAL Workshop 'The INTEGRAL Universe', Munich, 16-20 February 2004. Accepted for publication in ESA SP-552
dc.identifierhttps://arxiv.org/abs/astro-ph/0406399
dc.identifierhttp://arxiv.org/abs/astro-ph/0406399
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7855
dc.subjectAstrophysics
dc.titleINTEGRAL monitoring of the Black Hole candidate 1E 1740.7-2942
dc.typetext

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