Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-28T22:37:39.757Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectral Changes of Pleione - Start of a New Cycle?

Published online by Cambridge University Press:  12 April 2016

L. Iliev
L. Iliev*
Affiliation:
Institute of Astronomy and Bulgarian National Astronomical Observatory ”Rozhen”, 72 Tsarigradsko Shossee Blvd., BG-1784, Sofia, Bulgaria

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.

This is a preliminary report on spectral variability of Pleione during the present Be phase. The spectral activity of the star confirms the observed photometrical trend.

Type
6. Disks
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 566 - 568
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Hanuschik, R.W., Hummel, W., Dietle, O., Sutorius, E. 1995, A&A 300, 163 Google Scholar
Hanuschik, R.W., Hummel, W., Sutorius, E., Thimm, G. 1996, A&AS 116, 309 Google Scholar
Hummel, W. 1998, A&A 330, 243 Google Scholar
Iliev, L., Ruusalepp, M., Kovachev, B. 1988, Commis. 27 LAU Inf. Bull. Var.Stars No 3204Google Scholar
Iliev, L., Hoffmann, D., 1997, unpubl.Google Scholar
Sharov, A.S., Lyutyi, B.M. 1997, Pis’ma Astr. Zh. 23, No 2, 113 Google Scholar
Zorec, J. 1994, in IAU Symp. 162, Balona, L.A., H.F., Henrichs, J.M., Le Contel, Eds., Kluwer, p.362 Google Scholar