Hostname: page-component-848d4c4894-wg55d Total loading time: 0 Render date: 2024-05-17T12:16:44.622Z Has data issue: false hasContentIssue false

Asteroseismology of β Cep: Influence of Updated Microphysics

Published online by Cambridge University Press:  12 April 2016

H. Shibahashi
Affiliation:
Department of Astronomy, University of Tokyo, Japan
T. Koshikawa
Affiliation:
Department of Astronomy, University of Tokyo, Japan

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.

With updated microphysics such as opacity, we revise the result of asteroseismic investigations for β Cephei and show the tolerable range of the physical parameters of the star.

Type
Part 2.2. B-Type Stars
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Henrichs, H.F., et al. 1993, in New perspectives on stellar pulsation and pulsating variable stars, eds. Nemec, J. & Matthews, J., (Cambridge Univ. Press), 295 Google Scholar
Henrichs, H.F., et al. 2000, in Magnetic fields of chemically peculiar and related stars, eds. Glagolevskij, Y. & Romanyuk, I., 57 Google Scholar
Shibahashi, H. & Aerts, C. 2000, Apj, 531, L143 Google Scholar
Telting, J.H., Aerts, C., & Mathias, P. 1997, A&A, 322, 493 Google Scholar