CANGAROO III Observations of the Supernova Remnant RX J0852.0-4622
Sub-TeV gamma-ray emission from the northwest rim of the supernova remnant RX J0852.0-4622 was detected with the CANGAROO II telescope and recently confirmed by the HESS group. In addition, the HESS data revealed a very wide (up to 2° in diameter), shell
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|Source:||Astrophysical Journal, The|
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