SNR G330.2+1.0: A New Candidate Cosmic Ray Accelerator

Details SNR G330.2+1.0: A New Candidate Cosmic Ray Accelerator SNR G330.2+1.0: A New Candidate Cosmic Ray Accelerator

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1962g&link_type=abstract

Chandra Proposal ID #07500377

Physics

Chandra Proposal Id #07500377

Scientific paper

We propose to observe a Galactic supernova remnant (SNR) G330.2+1.0.
G330.2+1.0 is dominated by nonthermal X-ray emission from the shell, and
is thus a good candidate for a high energy cosmic ray acceleration site.

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