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Radial Velocity Variations in 69 Orionis
Published online by Cambridge University Press: 14 August 2015
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69 Ori (B5 V) was discovered as a Be star in 1976 (Doazan et al., 1977). We observed this object at the Merate Observatory during the periods Nov. 77. - Jan. 78 - Jan. 78 and Oct. 78 - Feb. 79 obtaining 20 red spectrograms and 25 blue ones with a dispersion of 35 Å/mm. We performed also B and V photo-electric observations during 12 nights altogether. The results from the red spectra and the photometric measurements have been discussed by Bossi et al. (1981).
- Type
- III. Spectroscopy
- Information
- Copyright
- Copyright © Reidel 1982
References
Bossi, M., Guerrero, G., Mantegazza, L., Rusconi, L., Scardia, M., Sedmak, G., 1981, Astron. Astrophys. Suppl., to be published.Google Scholar
Chandrasekhar, S., 1969, Ellipsoidal figures of equilibrium, Yale University Press, New Haven.Google Scholar
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