Observation of supernova remnants with the CAT Cherenkov imaging telescope

Details Observation of supernova remnants with the CAT Cherenkov imaging telescope Observation of supernova remnants with the CAT Cherenkov imaging telescope

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510...77m&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 77-81 (2000).

Computer Science

1

Supernova Remnants, Radiation Mechanisms, Polarization, Gamma-Ray

Scientific paper

Supernova remnants (SNR) can be broadly classified into two types: plerionic or plasma-filled SNR, like the Crab Nebula, and shell-type SNR, like Cassiopeia A (Cas A). VHE observations of the Crab Nebula and Cas A made with the CAT atmospheric Cherenkov imaging telescope are used to constrain models for production of gamma rays in SNR. For both plerionic and shell-type SNR, these observations serve primarily to impose a limit on the magnetic field in the region where the particles are accelerated. .

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