Circumstellar X-ray Emission from SN1978K

Details Circumstellar X-ray Emission from SN1978K Circumstellar X-ray Emission from SN1978K

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..553s&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 553-554

Astronomy and Astrophysics

Astrophysics

X-Rays, Circumstellar Matter, Supernovae

Scientific paper

We present the X-ray light curve in the 0.2 2.4 keV band based on
fiveROSAT observations of SN1978K in NGC 1313. The X-ray emission is
believed to arise from the interaction of the reverse shock and the
expanding debris from the supernova. The reverse shock becomes
established after the outgoing shock runs into circumstellar matter.

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