Models for X-ray emission from the A.D. 1006 supernova remnant

Details Models for X-ray emission from the A.D. 1006 supernova remnant Models for X-ray emission from the A.D. 1006 supernova remnant

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...211..562w&link_type=abstract

Astrophysical Journal, vol. 211, Jan. 15, 1977, pt. 1, p. 562-564. Research supported by Middlebury College

Astronomy and Astrophysics

Astrophysics

12

Astronomical Models, Shock Waves, Supernova Remnants, X Ray Sources, Detonation Waves, Gas Density, Interstellar Gas, Propagation Velocity, Radiant Flux Density

Scientific paper

The recently detected X-ray emission from the remnant of the A.D. 1006 supernova is interpreted in terms of blast-wave and reverse-shock models. It is found that while either model can provide a consistent explanation for the observations, the reverse-shock description leads to more reasonable values for the interstellar density and blast energy. Interestingly, both models indicate a distance of about 1.2 kpc for the remnant.

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