H I absorption in the direction of SS 433

Details H I absorption in the direction of SS 433 H I absorption in the direction of SS 433

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....82l...1v&link_type=abstract

Astronomy and Astrophysics, vol. 82, no. 3, Feb. 1980, p. L1, L2.

Astronomy and Astrophysics

Astronomy

21

Absorption Spectra, Emission Spectra, H Lines, Radio Sources (Astronomy), Supernova Remnants, Interstellar Extinction, Microwave Spectra, Radio Telescopes

Scientific paper

H I absorption has been observed in the direction of the unusual object SS 433 with the Westerbork Synthesis Radio Telescope. The H I data imply a lower limit of 3.7 kpc for the distance of SS 433 and a weak upper limit of 4.7 kpc. This agrees with the lower limit derived by Margon et al. (1979) based on observations of the interstellar NaD lines and is consistent with a physical association of SS 433 with the SNR W 50.

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