The X-ray Emission of SN1978K: Still Here After All These Years

Details The X-ray Emission of SN1978K: Still Here After All These Years The X-ray Emission of SN1978K: Still Here After All These Years

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21543002s&link_type=abstract

American Astronomical Society, AAS Meeting #215, #430.02; Bulletin of the American Astronomical Society, Vol. 42, p.356

Astronomy and Astrophysics

Astronomy

Scientific paper

SN1978K in NGC 1313 was observed by Suzaku in 2005 October for 32 ksec. We fit the spectrum with a two-temperature APEC model, obtaining a soft kT of 0.60 keV and a hard kT of 2.2 keV. The soft
0.5-2 keV band light curve shows that the apparent decrease described in 2003 is a dip and not a trend. Additional data will be presented from archival XMM observations. The X-ray emission from SN1978K appears to be as robust as ever.

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