X-ray structure of the Puppis supernova remnant

Details X-ray structure of the Puppis supernova remnant X-ray structure of the Puppis supernova remnant

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...207l.163c&link_type=abstract

Astrophysical Journal, vol. 207, Aug. 1, 1976, pt. 2, p. L163-L165. Research supported by the Lockheed Independent Research Pro

Computer Science

Sound

6

Radio Sources (Astronomy), Supernova Remnants, X Ray Sources, Angular Distribution, Astronomical Maps, Histograms, Rocket Sounding

Scientific paper

The angular distribution of X-ray emission from the Puppis supernova remnant was investigated with a focusing X-ray collector during a rocket observation. Extent of the X-ray emitting region along the direction of scan is 42 (+ or - 4) arcmin and is well correlated with the size of the Puppis A radioshell. The existence of a feature within the remnant is confirmed whose X-ray emission is strongly localized, and its spectrum is observed to be softer than the rest of the remnant.

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