Monitoring of SN 1987A

Details Monitoring of SN 1987A Monitoring of SN 1987A

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..260g&link_type=abstract

Chandra Proposal ID #01500038

Physics

Chandra Proposal Id #01500038

Scientific paper

Over the next decade, the shock front from the supernova explosion SN 1987A in the Large Magellanic Cloud will interact with a comlex environment. The X-ray emission is likely to brighten and change in various ways as the shock encounters the dense ring, HII region and red giant wind. Regular monitoring of the source throughout the duration of the AXAF mission is needed to test models of remnant evolution, nonequilibrium ionization processes and elemental abundances.

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