no code implementations • 26 Jan 2021 • J. Rodi, A. Tramacere, F. Onori, G. Bruni, C. Sánchez-Fernández, M. Fiocchi, L. Natalucci, P. Ubertini
Spectral analysis of the hard X-rays found a \(kT_e \sim 30 \) keV and \( \tau \sim 2\) with a \texttt{CompTT} model, indicative of an accreting black hole binary in the hard state.
High Energy Astrophysical Phenomena