Spectrum of the supernova remnant W50

Details Spectrum of the supernova remnant W50 Spectrum of the supernova remnant W50

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.190p..65m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 190, Mar. 1980, p. 65P-68P.

Other

7

Emission Spectra, Line Spectra, Stellar Spectrophotometry, Supernova Remnants, Interstellar Extinction, Nebulae, Radial Velocity, X Ray Sources

Scientific paper

Nebulosity associated with the supernova remnant W50 is collisionally excited ([S II]/Hα ˜ 2), highly reddened (AV = 4.5) and has a large radial velocity (166 km s-1) It also has abnormally strong [N II] lines ([N II]/Hα ˜ 5), Puppis-A being the only other supernova remnant showing such an anomaly. The large reddening is not inconsistent with the suggestion that the peculiar emission-line object and X-ray source SS433 is associated with W50.

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