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[ascl:2207.020] vKompth: Time-dependent Comptonization model for black-hole X-ray binaries

vKompth fits the energy-dependent rms-amplitude and phase-lag spectra of low-frequency quasi-periodic oscillations in low mass black-hole X-ray binaries using a variable Comptonization model. The accretion disc is modeled as a multi-temperature blackbody source emitting soft photons which are then Compton up-scattered in a spherical corona, including feedback of Comptonized photons that return to the disc.

Code site:
https://github.com/candebellavita/vkompth
Described in:
https://ui.adsabs.harvard.edu/abs/2022MNRAS.515.2099B
Bibcode:
2022ascl.soft07020B

Views: 1262

ascl:2207.020
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