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Comptonization in 1E 1740.7-2942 spectra from 2 to 200 keV

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.

preprint2013arXivOpen access
Manuel CastroTaís MaiolinoFlavio D'AmicoJörn WilmsKatja PottschmidtJoão Braga
astro-ph.HE
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Open access6 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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Manuel CastroTaís MaiolinoFlavio D'AmicoJörn WilmsKatja PottschmidtJoão Braga

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