Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-17T17:20:35.096Z Has data issue: false hasContentIssue false
  • English
  • Français

Asteroseismology of the β Cephei Variable 16 (EN) Lacertae

Published online by Cambridge University Press:  12 April 2016

W.A. Dziembowski  and
M. Jerzykiewicz
W.A. Dziembowski
Affiliation:
Copernicus Astronomical Centre, Polish Academy of Sciences ul. Bartycka 18, 00-716 Warsaw, Poland
M. Jerzykiewicz
Affiliation:
Wroclaw University Observatory ul. Kopernika11, 51-622 Wroclaw, 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.

Various observational data and model calculations are used to identify four pulsation modes detected in this star and to infer its properties. It is concluded that the star’s interior must rotate faster than the outer layers.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 289 - 290
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Cugier, H., Dziembowski, W.A., & Pamyatnykh, A.A. 1994, A&A, 291, 143 Google Scholar
Dziembowski, W.A., & Pamyatnykh, A.A. 1993, MNRAS, 262, 204 Google Scholar
Jerzykiewicz, M. 1993, Acta astr., 43, 13 Google Scholar