XMM and INTEGRAL Simultaneous Observations of 1E 1740.7-2942
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Author/Creator ORCID
Date
2013-07-18
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Citation of Original Publication
Castro, Manuel Avila, Taís Maiolino, Flavio D’Amico, Joern Wilms, Katja Pottschmidt, and João Braga. “XMM and INTEGRAL Simultaneous Observations of 1E 1740.7-2942.” In Proceedings of An INTEGRAL View of the High-Energy Sky (the First 10 Years) - 9th INTEGRAL Workshop and Celebration of the 10th Anniversary of the Launch — PoS(INTEGRAL 2012), 176:046. SISSA Medialab, 2013. https://doi.org/10.22323/1.176.0046.
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Attribution-NonCommercial-ShareAlike 1.0 Generic (CC BY-NC-SA 1.0)
Attribution-NonCommercial-ShareAlike 1.0 Generic (CC BY-NC-SA 1.0)
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Abstract
Studies of the long-term spectral variations have been used to constrain the emission processes
of black hole candidates. However, a common scenario which is able to explain the emission
from soft to hard X-rays has been proposed only recently. Here, we use XMM and INTEGRAL
data on 1E 1740.7−2942 in order to demonstrate that Comptonization plays an important role in
producing high energy photons, as predicted by the current modeling scenario.