The mass loss from the O 9.5 Ib supergiant, zeta Orionis, derived from the H-alpha profile

Details The mass loss from the O 9.5 Ib supergiant, zeta Orionis, derived from the H-alpha profile The mass loss from the O 9.5 Ib supergiant, zeta Orionis, derived from the H-alpha profile

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....40..277h&link_type=abstract

Astronomy and Astrophysics, vol. 40, no. 3, May 1975, p. 277-283. Research sponsored by the Deutsche Forschungsgemeinschaft.

Astronomy and Astrophysics

Astrophysics

66

B Stars, H Alpha Line, O Stars, Stellar Spectra, Stellar Winds, Supergiant Stars, Astronomical Models, Mass Transfer, Spectral Line Width, Stellar Mass Ejection, Ultraviolet Spectra

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1975A&A....40..277H

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