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Profils de la raie Hα par television analogique
Published online by Cambridge University Press: 12 April 2016
Summary
High resolution profiles of the Hα line are derived for about thirty Be stars and several bright stars by means of the anological television system. The profiles obtained with this method fairly agree with the theoretical ones (a Lyrae).
- Type
- Session I - Winds from Early Type Stars: Observations
- Information
- International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 57 - 60
- Copyright
- Copyright © Reidel 1981
References
- 2
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