Hostname: page-component-6bf8c574d5-k2jvg Total loading time: 0 Render date: 2025-03-07T08:35:16.959Z Has data issue: false hasContentIssue false
  • English
  • Français

The photosphere of Pleione(*)

Published online by Cambridge University Press:  26 May 2016

J. Zorec
J. Zorec*
Affiliation:
Institut d'Astrophysique de Paris - 98bis, Bd. Arago, 75014 Paris

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.

In this paper we report results concerning the photospheric Balmer discontinuity of Pleione. They show that after the Be → Be-shell phase transitions, the stellar photosphere keeps its characteristics unchanged.

Type
6. Be Stars: Circumstellar Environment
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 362 - 363
Copyright
Copyright © Kluwer 1994 

References

Divan, L.: 1979, in McCarty, M.F., Coyne, G.V., Philip, A.G.D., ed(s)., Spectral Classification in the Future , IAU Coll. 47, 247 CrossRefGoogle Scholar
Divan, L., Zorec, J.: 1982, The Hipparcos Space Mission , ESA SP-177, 101 Google Scholar
Johnson, H.L., Mitchel, R.I., Iriarte, B., Wisniewski, W.Z.: 1966, Lun. Plan. Lab. 4, 99 Google Scholar
Johnson, H.L., Mitchel, R.I., Latham, A.S.: 1967, Lun. Plan. Lab. 6, 85 Google Scholar
Sharov, A.S., Lyutiy, B.M.: 1972, IAU Inf. Bull. Var. Stars , 698 Google Scholar
Zorec, J.: 1986, Thèse d'Etat , Universite Paris VII Google Scholar
Zorec, J., Höflich, P., Divan, L.: 1989, Astron. Astrophys. 210, 279 Google Scholar
Zorec, J., Briot, D.: 1991, Astron. Astrophys. 245, 150 Google Scholar