Radio and optical observations of SS 433

Details Radio and optical observations of SS 433 Radio and optical observations of SS 433

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84.1037s&link_type=abstract

Astronomical Journal, vol. 84, July 1979, p. 1037-1041. Research supported by the National Science and Engineering Research Cou

Astronomy and Astrophysics

Astronomy

36

Emission Spectra, Optical Emission Spectroscopy, Radio Astronomy, Radio Sources (Astronomy), Variable Stars, Balmer Series, H Beta Line, Optical Polarization, Radiant Flux Density, Stellar Spectra, Supernova Remnants, Tables (Data), X Ray Sources

Scientific paper

Results are presented for radio and limited optical spectroscopic observations of the peculiar emission variable star SS 433, which appears to be associated with the X-ray source A1909+04 and the supernova remnant W50. The radio source is nonthermal and shows clear evidence for variability on a time scale as short as a few hours. Neither linear nor circular polarization was detected. The optical spectra indicate intense Balmer and other lines superimposed on a red continuum, with evidence for variability in the H-beta profile. The significance of these observations is briefly discussed.

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