Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-12-01T08:57:47.529Z Has data issue: false hasContentIssue false
  • English
  • Français

Observation de la Raie Hα dans les Etoiles Be

Published online by Cambridge University Press:  14 August 2015

Y. Andrillat  and
Ch. Fehrenbach
Y. Andrillat
Affiliation:
Observatoire de Haute Provence
Ch. Fehrenbach
Affiliation:
Observatoire de Haute Provence

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 135 - 139
Copyright
Copyright © Reidel 1982 

References

Adrianzyk, G., Baietto, J.C., Berger, J.P., Fehrenbach, Ch., Prévot, L., Vin, A.: 1978, Astron. Astrophys. 63, 279.Google Scholar
Andrillat, Y., Fehrenbach, Ch.: 1981a, Coll. UAI n°59.CrossRefGoogle Scholar
Andrillat, Y., Fehrenbach, Ch.: 1981b, 2° Colloque National du Comité Français du Télescope Spatial.Google Scholar
Jaschek, M., Hubert-Delplace, A.M., Hubert, H., Jaschek, C.: 1980, Astron. Astrophys. Suppl. Ser. 42, 113.Google Scholar
Kurucz, L.: 1979, Astrophys. J. Suppl. 40, 1.CrossRefGoogle Scholar
Slettebak, A., Reynolds, R.C.: Astrophys. J. Suppl. Ser. 38, 205.CrossRefGoogle Scholar