Abstracts, Galactic Center Workshop '98
GCNEWS
A Newsletter for Galactic Center Research
This Volume was edited by Angela Cotera & Heino Falcke
email: gcnews@aoc.nrao.edu

ABSTRACT

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Explaining the spectrum of Sgr A* using a two temperature plasma
Rohan Mahadevan
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, England.
ABSTRACT:
Recently Narayan et al. (1998) have used an advection dominated
accretion flow (ADAF) model to explain the low luminosity and spectrum
from Sgr A*. This model explains the millimeter to hard X-ray
spectrum quite well, but has had difficulty in agreeing with the low
energy radio observations. An essential element of the model is that
the thermal electrons must co-exist with hot (nearly virial) protons
throughout the flow. Until now, this two temperature nature has been
little more than theoretical speculation. We show that an emission
process associated with the protons naturally resolves the observed
discrepancy and low radio energies. In particular, the hot protons
produce charged pions which subsequently decay into electrons and
positrons. These high energy particles interact with the local
magnetic fields to produce synchrotron radiation which naturally
reproduces the observed spectral break at ~ 86 GHz as well as the
low energy radio spectrum. No fine tuning of the model is allowed.
This provides observational support for both a two temperature plasma, and
a power-law energy distribution of protons.
Further, it gives increasing support to the idea that
Sgr A* most probably accretes via an ADAF.
LINKS: Program, Author, rohan@ast.cam.ac.uk
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