Soft X-ray emission in Eridanus - an old supernova remnant

Details Soft X-ray emission in Eridanus - an old supernova remnant Soft X-ray emission in Eridanus - an old supernova remnant

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...208..718n&link_type=abstract

Astrophysical Journal, vol. 208, Sept. 15, 1976, pt. 1, p. 718-726.

Astronomy and Astrophysics

Astrophysics

40

Astronomical Spectroscopy, Supernova Remnants, X Ray Sources, H Lines, Hydrogen Clouds, Oxygen Spectra, Pulsars, Radio Stars, Spectrum Analysis

Scientific paper

Data are presented on the soft X-ray intensity and spectrum of a region of extended emission in the constellation Eridanus. This region also includes optical filaments, the hard X-ray source 3U 0431-10, the radio pulsar MP 0450, a neutral hydrogen shell structure, and an O VI absorption feature. It is suggested that these features are all part of an old supernova remnant with an age in the range from 100,000 to 1 million yrs.

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