Images of Two Component Advective Flow around Black Holes in presence of outflows and cooling
Abstract
In the literature, several authors have presented images of black holes surrounded by Keplerian disks or simple one component disks. However, successful fitting of the spectral and timing properties suggest that the disks around black hole are of two components, one Keplerian and the other sub-Keplerian. We present images, spectra and energy dependent time lags of Two Component Advective Flow. Hydrodynamical configuration of low angular momentum, sub-keplerian component is generated by the Total Variation Diminishing (TVD) method. To produce the spectra, we incorporate Comptonization via Monte-Carlo technique. The spectral energy distribution, images over various inclination angles on observer plane are obtained by Ray-Tracing process. Variations caused by the self consistent outflows are reported.
- Publication:
-
42nd COSPAR Scientific Assembly
- Pub Date:
- July 2018
- Bibcode:
- 2018cosp...42E.588C