Radio emission from CYG OB 2 No. 12

Details Radio emission from CYG OB 2 No. 12 Radio emission from CYG OB 2 No. 12

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....92l...5w&link_type=abstract

Astronomy and Astrophysics, vol. 92, no. 1-2, Dec. 1980, p. L5, L6.

Astronomy and Astrophysics

Astronomy

10

B Stars, Early Stars, O Stars, Radio Astronomy, Radio Stars, Stellar Mass Ejection, Supergiant Stars, Stellar Luminosity, Stellar Radiation, Stellar Winds

Scientific paper

Radio emission of the star No. 12 of the Cygnus OB 2 association has been detected. It is discussed in terms of the rate of mass loss. The rate is still compatible with current understanding of a fast line- driven stellar wind of early type stars, even at this rather late spectral type and very high luminosity. It seems to indicate that for evolved stars the strength of this wind may be independent of spectral type.

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