SS433 - A massive black hole

Details SS433 - A massive black hole SS433 - A massive black hole

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979natur.278..719t&link_type=abstract

Nature, vol. 278, Apr. 19, 1979, p. 719, 720.

Astronomy and Astrophysics

Astrophysics

12

Black Holes (Astronomy), Emission Spectra, Stellar Spectra, Astrophysics, Balmer Series, Doppler Effect, H Alpha Line, H Beta Line, Stellar Mass Accretion, X Rays

Scientific paper

Anomalous emission lines from the object SS433 may be explained by an emitting ring of gas in a circular orbit around a central, massive black hole. The broad, strong anomalous emission lines move rapidly across the spectrum; two such movements, when interpreted as Doppler shifts, imply velocity changes of 6000 and -3500 km/sec. Accretion onto the massive black hole may account for the optical continuum radiation, broad emission lines, weak radio and X-ray emission from SS433.

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