Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-20T00:14:22.682Z Has data issue: false hasContentIssue false
  • English
  • Français

How May Seismological Measurements Constrain Parameters of Stellar Structure?

Published online by Cambridge University Press:  12 April 2016

Timothy M. Brown ,
Jørgen Christensen-Dalsgaard  and
Barbara W. Mihalas
Timothy M. Brown
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307, USA
Jørgen Christensen-Dalsgaard
Affiliation:
Institute of Physics and Astronomy, Aarhus University, Aarhus, DK
Barbara W. Mihalas
Affiliation:
National Center for Supercomputing Applications, 605 E. Springfield Ave., Urbana, IL 61820, USA

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.

Pulsation frequency separations, combined with other observations, can constrain the structural parameters of Sun-like stars. As an example, we treat a hypothetical visual binary system resembling α Cen.

Type
VI. Asteroseismology: theory
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 554 - 556
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Christensen-Dalsgaard, J. 1988, In Advances in Helio- and Asteroseismology, eds Christensen-Dalsgaard, J. and Frandsen, S., Reidel, D., Dordrecht, p. 295.Google Scholar
Gough, D.O. 1987, Nature 326, 257.Google Scholar
Ulrich, R.K. 1986, Ap. J. 306, L37.Google Scholar