Soft X-ray emission from the Lupus Loop and SN 1006 supernova remnants

Details Soft X-ray emission from the Lupus Loop and SN 1006 supernova remnants Soft X-ray emission from the Lupus Loop and SN 1006 supernova remnants

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...229l.123w&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 229, May 1, 1979, p. L123-L128. Research supported by the Research C

Astronomy and Astrophysics

Astrophysics

19

Nebulae, Supernova Remnants, X Ray Sources, X Ray Spectra, Brightness Temperature, Neutron Stars, Raster Scanning, Sas-3

Scientific paper

X-ray maps of the Lupus region have been obtained in a raster scan observation from SAS 3. These show the Lupus Loop to be a faint extended source of soft X-rays with a temperature about 2.5 million K. The most prominent feature of the region is the A.D. 1006 supernova remnant, which is unexpectedly bright at 0.2-1.0 keV. One speculative interpretation of the low-energy flux from SN 1006 is as blackbody radiation from a hot neutron star.

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