SS433 - Mystery star

Details SS433 - Mystery star SS433 - Mystery star

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980newsc..85..248c&link_type=abstract

New Scientist, vol. 85, Jan. 24, 1980, p. 248-251.

Astronomy and Astrophysics

Astronomy

1

Stellar Mass Ejection, Supernova Remnants, X Ray Sources, Annual Variations, Black Holes (Astronomy), Helium, Line Spectra, Radio Astronomy, Spectrum Analysis, Stellar Models

Scientific paper

Continuing observations support the theory that SS433 is ejecting matter at speeds a quarter of that of light, speeds much higher than for any other object in the Galaxy. This paper reviews data on SS433, including a radio map of the supernova remnant W50, the spectrum of SS433, and the variation in the wavelength of the moving spectral lines of the object. It is suggested that SS433 is a new type of supernova remnant, that is, a remnant that is not a pulsar.

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