Soft X-rays from very young supernova remnants

Details Soft X-rays from very young supernova remnants Soft X-rays from very young supernova remnants

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.205..303b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 205, Oct. 1983, p. 303-308.

Astronomy and Astrophysics

Astronomy

3

Stellar Models, Supernova Remnants, X Ray Sources, Dynamic Models, Emission Spectra, Stellar Mass Ejection

Scientific paper

A dynamical model of the very early evolution of a supernova remnant suggests that copious emission of X-rays will occur in the first 10 years. The radiation is largely in spectral lines in the range from 20 to 50 Å and will be most easily observable towards the end of the first decade. The effect should be detectable, using state-of-the-art instruments, in any supernova occurring within 23 Mpc.

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