A soft X-ray survey of galactic supernova remnants with the Einstein Observatory

Details A soft X-ray survey of galactic supernova remnants with the Einstein Observatory A soft X-ray survey of galactic supernova remnants with the Einstein Observatory

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phdt.........4p&link_type=abstract

Ph.D. Thesis Columbia Univ., New York, NY.

Computer Science

Heao 2, Interstellar Matter, Supernova Remnants, X Ray Spectra, Hydrogen, Line Spectra, Luminosity, Morphology, Plasma Temperature, Thermal Emission

Scientific paper

The Einstein Observatory was used to observe 19 galactic supernova remnants in the soft X-ray band. The X-ray luminosities and X-ray morphologies of the remnants were then compared to optical and radio data, with some large scale correlation between the radio and X-ray features noted in several of the remnants. The temperature of the emitting X-ray plasma was obtained through a spectral analysis of each remnant in the sample. Detailed analyses were carried out on the two remnants representing the extremes in age.

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