X-ray spectra of the Cassiopeia A and TYCHO supernova remnants and their element abundances

Astronomy and Astrophysics – Astrophysics

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Abundance, Supernova Remnants, X Ray Spectra, Bremsstrahlung, Emission Spectra, Line Spectra, Proportional Counters, Scintillation Counters, Stellar Models

Scientific paper

X-ray spectra of the supernova remnants Cas A and Tycho were obtained with the gas scintillation proportional counters on board Tenma. The observed spectra can be well fitted with single thermal bremsstrahlung continuum spectra with several emission features due to line blends of silicon, sulfur, argon, calcium, and iron. The mean energies of these line blends cannot be accounted for by invoking an equilibrium ionization model, but a simple, nonequilibrium model gives agreement with the data. In particular, the mean energy of each of the five line blends implies a value for the ionization time scale (the product of the electron density and time) of 1.0 × 1011 cm-3 s and 6.0 × 109 cm-3 s for Cas A and for Tycho respectively. The line intensities compared with those predicted by the nonequilibrium model give the element abundances in these objects. The results support current models of Type I and Type II supernovae.

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