X-ray maps of the VELA supernova remnant

Details X-ray maps of the VELA supernova remnant X-ray maps of the VELA supernova remnant

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235l..67h&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 235, Jan. 15, 1980, p. L67-L69.

Astronomy and Astrophysics

Astronomy

3

Astronomical Maps, Supernova Remnants, X Ray Astronomy, X Ray Imagery, Image Processing, Radio Sources (Astronomy), Sas-3, Wiener Filtering

Scientific paper

X-ray maps of the Vela supernova remnant in two energy channels, 0.1-0.4 keV and 0.4-0.8 keV, are presented. The data were obtained in 1975 from a SAS 3 satellite observation. We describe the Wiener filter technique used to deconvolve the angular response of the instrument from the data. The X-ray structure is compared with the optical and radio features of the region.

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