Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-24T05:57:55.529Z Has data issue: false hasContentIssue false
  • English
  • Français

Stability of the pulsation of 12 (DD) Lacertae

Published online by Cambridge University Press:  26 May 2016

A. Pigulski
A. Pigulski*
Affiliation:
Astronomical Institute, Wrocław University, Kopernika 11, 51-622 Wrocław, Poland

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.

The results of the study of period changes of all pulsational components in the multiperiodic β Cephei-type star, 12 Lac, are summarized.

Type
1. Pulsation and Rotation
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 21 - 22
Copyright
Copyright © Kluwer 1994 

References

Ciurla, T.: 1987, Acta Astronomica 37, 53 Google Scholar
Jerzykiewicz, M.: 1978, Acta Astronomica 28, 465 Google Scholar
Shobbrook, R.R.: 1973, M.N.R.A.S. 161, 257 Google Scholar
Smith, M.A.: 1980, Ap.J. 240, 149 Google Scholar