Spectral Properties of M87 Using Two-Component Flow

Details Spectral Properties of M87 Using Two-Component Flow Spectral Properties of M87 Using Two-Component Flow

2009-03-09

arxiv.org/abs/0903.1549v1

AIP Conf.Proc.1053:29,2008

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

4 Pages, 1 Figures, Proceeding of the 2nd Kolkata Conference on "Observational Evidence for the Black Holes in the Universe",

Scientific paper

10.1063/1.3009499

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.

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