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 (α Lyrae).
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References
Fehrenbach, Ch., Vin, A.: 1975, Image Processing Techniques in Astronomy, D. Reidel Publ. Cy, pp. 109–116.
Adrianzyk, G., Baietto, J. C., Berger, J. P., Fehrenbach, Ch., Prévot, L., Vin, A.: 1978, Astron. Astrophys. 63, pp. 279–283.
Kurucz, L.: 1979, Ap. J. Suppl. 40, pp. 1–340.
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© 1981 D. Reidel Publishing Company
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Andrillat, Y., Fehrenbach, C. (1981). Profils De La Raie Hα Par Television Analogique. In: Chiosi, C., Stalio, R. (eds) Effects of Mass Loss on Stellar Evolution. Astrophysics and Space Science Library, vol 89. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-8500-1_9
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DOI: https://doi.org/10.1007/978-94-009-8500-1_9
Publisher Name: Springer, Dordrecht
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