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UV and Radiofrequency Observations of Wolf-Rayet Stars

Published online by Cambridge University Press:  14 August 2015

Hugh M. Johnson
Hugh M. Johnson*
Affiliation:
Lockheed Missiles and Space Company, Palo Alto, Calif., U.S.A.

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Very few observations are available. Of early rocket work on γ Vel (Stecher and Milligan, 1962; Smith, 1967) the most detailed spectra are by Stecher (1968) in the range λ 1200–3100 Å and by Carruthers (1968) in the range λ 1050–1216 Å. West's (1971) spectrum of γ Vel with the OAO-2 spectrometer (Code et al., 1970) in the range λ 1050–2000 Å appears to be somewhat different from Stecher's. Comparison must await full details.

Type
Section II
Information
Symposium - International Astronomical Union , Volume 49: Wolf-Rayet and High Temperature Stars , 1973 , pp. 42 - 53
Copyright
Copyright © Reidel 1973 

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