Spectral Properties of M87 Using Two-Component Flow
High Energy Astrophysical Phenomena
2010-12-13 v1
Abstract
We fit the observational data for M87 using two-component advective disk model. We show that the flat spectrum from the nucleus of M87 is due to synchrotron radiation produced by non-thermal electrons in the CENBOL. The non-thermal distribution is produced due to acceleration of electrons across the shock in a sub-Keplerian flow.
Cite
@article{arxiv.0903.1549,
title = {Spectral Properties of M87 Using Two-Component Flow},
author = {Samir Mandal},
journal= {arXiv preprint arXiv:0903.1549},
year = {2010}
}
Comments
4 Pages, 1 Figures, Proceeding of the 2nd Kolkata Conference on "Observational Evidence for the Black Holes in the Universe", Published in AIP, 2008