no code implementations • 9 Feb 2021 • F. Cangemi, T. Beuchert, T. Siegert, J. Rodriguez, V. Grinberg, R. Belmont, C. Gouiffès, I. Kreykenbohm, P. Laurent, K. Pottschmidt, J. Wilms
We discuss the potential origins of the high-energy components in both states, and favor an interpretation where the part of the high-energy component is due to a compact jet in the hard state and hybrid Comptonization in either a magnetised or non-magnetised corona in the soft state.
High Energy Astrophysical Phenomena
no code implementations • 8 Aug 2020 • M. Cruces, L. G. Spitler, P. Scholz, R. Lynch, A. Seymour, J. W. T. Hessels, C. Gouiffès, G. H. Hilmarsson, M. Kramer, S. Munjal
We model the bursts cumulative energy distribution, with energies from ${\sim}10^{38}$-$10^{39}$ erg, and find that it is well described by a power-law with slope of $\gamma=-1. 1\pm 0. 2$.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics