no code implementations • 2 Feb 2021 • F. Onori, M. Fiocchi, N. Masetti, A. F. Rojas, A. Bazzano, L. Bassani, A. J. Bird
The new INTEGRAL and Swift data collected during the 2019 X-ray outburst of Swift J1713. 4-4219, in combination with the archival optical/NIR observations, suggest a LMXB classification for this source.
High Energy Astrophysical Phenomena
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
