The X-ray Emission from Old Supernovae

Details The X-ray Emission from Old Supernovae The X-ray Emission from Old Supernovae

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cxo..prop.1465s&link_type=abstract

Chandra Proposal ID #05500627

Computer Science

Chandra Proposal Id #05500627

Scientific paper

We propose to observe several supernovae that for which the expected flux remains high. Several sources discovered in past years using Einstein, ROSAT, or ASCA are still emitting at high luminosities; a measurement of the expected enhanced metallicity in SN1988Z will test the compact SNR model. For SN1979C, the temperature should still be high, yet a short ACIS observation placed only an upper limit on the emission. A modest observation of SN1982aa will leverage ROSAT data, yielding a light curve.

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