Spectral Properties of M87 Using Two-Component Flow

Samir Mandal

doi:10.1063/1.3009499

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arXiv · 0903.1549

Spectral Properties of M87 Using Two-Component Flow

Samir Mandal

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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.

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Samir Mandal. 2009-03-09. Spectral Properties of M87 Using Two-Component Flow. https://doi.org/10.1063/1.3009499

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