A New Emulated Monte Carlo Radiative Transfer Disk-Wind Model: X-Ray Accretion Disk-wind Emulator -- XRADE

We present a new X-Ray Accretion Disk-wind Emulator (\textsc{xrade}) based on the 2.5D Monte Carlo radiative transfer code which provides a physically-motivated, self-consistent treatment of both absorption and emission from a disk-wind by computing the local ionization state and velocity field with...

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Veröffentlicht in:	arXiv.org 2022-07
Hauptverfasser:	Matzeu, G A, Lieu, M, Costa, M T, Reeves, J N, Braito, V, Dadina, M, Nardini, E, Boorman, P G, Parker, M L, Sim, S A, Barret, D, Kammoun, E, Middei, R, Giustini, M, Brusa, M, J Pérez Cabrera, Marchesi, S
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Artificial neural networks Emulators Interpolation Luminosity Machine learning Physics - Astrophysics of Galaxies Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Quasars Radiative transfer Ray tracing Velocity distribution X ray spectra X-ray astronomy
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