Hard X-ray variability of V404 Cygni during the 2015 outburst
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DOI: 10.1051/0004-6361/201629620
Abstract: Aims. Hard X-ray spectra of black hole binaries (BHB) are produced by Comptonization of soft seed photons by hot electrons near the black hole. The slope of the resulting ray spectra is governed by two… read more here.
Keywords: hard ray; v404 cyg; v404; 2015 outburst ... See more keywords