X-ray line emission from the TYCHO supernova remnant

Details X-ray line emission from the TYCHO supernova remnant X-ray line emission from the TYCHO supernova remnant

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...8012987p&link_type=abstract

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Mathematics

Spectrum Analysis, Supernovae, X Ray Sources, X Ray Spectra, X Rays, Iron, Mathematical Models, Potassium, Silicon, X Ray Spectroscopy

Scientific paper

The observation of the X-ray spectrum of the Tycho supernova remnant in the energy range 0.5 to 20 keV is discussed. Four significant line features in the spectrum: The K alpha lines of silicon, sulphur, and iron; and the L lines of iron are examined. Comparisons between the silicon and sulphur equivalent widths and K alpha iron line energies of Tycho and Cas A are discussed. Suggest that the X-ray emitting plasma in Tycho is further from collisional ionization equilibrium than that of Cas A.

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