Spectral Properties of a Two Component and Two Temperature Advective Flow
Astrophysics
2016-11-09 v1
Abstract
Low angular momentum accretion flows very often have centrifugal pressure supported standing shock waves which can accelerate flow particles. The accelerated particles in turn emit synchrotron radiation in presence of magnetic fields. Efficient cooling of the electrons reduces its temperature in comparison to the protons. In this paper, we assume two temperature flows to explore this property of shocks and present an example of the emitted radiation spectrum.
Cite
@article{arxiv.astro-ph/0501292,
title = {Spectral Properties of a Two Component and Two Temperature Advective Flow},
author = {Samir Mandal and Sandip K. Chakrabarti},
journal= {arXiv preprint arXiv:astro-ph/0501292},
year = {2016}
}
Comments
4 pages, 2 figures To be published in the Proceedings of 10th Marcel Grossman Meeting, Ed. R. Ruffini et al. (World Scientific: Singapore)