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[ascl:2010.015] relxill: Reflection models of black hole accretion disks

relxill self-consistently connects an angle-dependent reflection model constructed with XILLVER (http://www.srl.caltech.edu/personnel/javier/xillver/index.html) with the relativistic blurring code RELLINE (ascl:1505.021). It calculates the proper emission angle of the radiation at each point on the accretion disk and then takes the corresponding reflection spectrum into account.

Code site:
http://www.sternwarte.uni-erlangen.de/~dauser/research/relxill/index.html https://github.com/thdauser/relxill
Described in:
https://ui.adsabs.harvard.edu/abs/2014ApJ...782...76G https://ui.adsabs.harvard.edu/abs/2014MNRAS.444L.100D https://ui.adsabs.harvard.edu/abs/2016A%26A...590A..76D
Bibcode:
2020ascl.soft10015D

Views: 211

ascl:2010.015
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