X-ray spectroscopic observations and modeling of supernova remnants

Details X-ray spectroscopic observations and modeling of supernova remnants X-ray spectroscopic observations and modeling of supernova remnants

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981xras.nasa..107s&link_type=abstract

In NASA. Goddard Space Flight Center X-ray Astronomy in the 1980's p 107-117 (SEE N82-26055 16-88)

Astronomy and Astrophysics

Astronomy

1

Abundance, Stellar Spectra, Supernova Remnants, X Ray Spectra, X Ray Spectroscopy, Black Holes (Astronomy), Neutron Stars, Plasmas (Physics), Spectrometers, Spectroscopic Analysis, Stellar Mass Ejection, X Ray Astronomy

Scientific paper

The X-ray observations of young remnants and their theoretical interpretation are described. A number of questions concerning the nature of the blast wave interaction with the interstellar gas and grains and of atomic processes in these hot plasmas are considered. It is concluded that future X-ray spectrometers with high collecting area, moderate spectral resolution and good spatial resolution can make important contributions to the understanding of supernova remnants in the Milky Way and neighboring galaxies and of their role in the global chemical and dynamical evolution of the interstellar medium.

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