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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Gamma-rays from the Galactic Center: A Point-Like or Diffuse Source?
Markoff, S.; Melia, F.; Sarcevic, I.
Physics Dept., Univ. Arizona
ABSTRACT:
Recently, EGRET onboard NASA telescope Compton GRO detected gamma-rays
from the Galactic Center (GC). The data can be fit by a power-law of
spectral index roughly 1.7, but the nature of the source of these
photons is still a matter of debate. While some groups favor the
massive black hole candidate Sgr A*, others postulate a diffuse
source. The lack of variability in the flux seems to suggest the
latter, but recent hydrodynamical simulations of the accretion process
indicate that the fluctuations may be below the detection level of the
current observations. Until instruments with the capability to resolve
the details of this region in the extreme high-energy evolve, we are
left to determine the source by identifying the most likely candidates
and attempting to model their spectra based on what we know of their
physical environments. In this talk I will present the results of our
model for Sgr A*. Having completed a detailed treatment of photon
production by hadronic collisions and other processes, we can now
begin to draw firm conclusions about whether or not the broadband
spectrum from this process in an accreting black hole environment is
consistent with the data.
LINKS: Program, Author, sera@physics.arizona.edu
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File last modified on Monday 04 August 2003 [10:43 MDT].
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