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Observation de la Raie Hα dans les Etoiles Be
Published online by Cambridge University Press: 14 August 2015
Abstract
Few studies concern the H alpha profile of the Be stars and it is difficult to do a fine analysis of the line structure, and of its variations from the results obtained with different resolutions and accuracies.
Then, it was useful to apply modern technics for the observation of this line to get an homogeneous material, sensitive enough to show fast variations of the order of few minutes because an accurate photometry is available using linear response receivers.
- Type
- III. Spectroscopy
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- Copyright © Reidel 1982
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