Gamma-ray Models for SN 1006 Using Different Astronomical Parameters

Details Gamma-ray Models for SN 1006 Using Different Astronomical Parameters Gamma-ray Models for SN 1006 Using Different Astronomical Parameters

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..281k&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astronomy

Supernova Remnants, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

We use nonlinear kinetic theory of cosmic ray acceleration in supernova remnants to study the properties of the nonthermal emission from SN 1006. The range of physical parameters is examined in order to find out whether it encompasses the existing data. It is shown that the γ-ray flux is very sensitive to the ambient gas density NH and that the existing H.E.S.S. upper limit requires NH <= 0.1 cm-3.

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