X-ray emission from the supernova remnants W 63 and HB 21

Details X-ray emission from the supernova remnants W 63 and HB 21 X-ray emission from the supernova remnants W 63 and HB 21

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..508b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, June 1989, p. 508-512. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Nebulae, Supernova Remnants, X Ray Sources, Astronomical Maps, Background Radiation, Flux Quantization, X Ray Imagery

Scientific paper

Using archival data of the Einstein Observatory, X-ray emission from W 63 and HB 21 were found with confidence levels of 7sigma and 5sigma, respectively. For both nebulae, the brightest parts of the X-ray images are the central ones. The X-ray fluxes and luminosities are determined. Two point X-ray sources were found near W 63; the first was the KO111 star BS 7798, while the second was not identified.

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