Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-30T00:56:37.605Z Has data issue: false hasContentIssue false
  • English
  • Français

A Hertzsprung-Russell diagram for stellar oscillations

Published online by Cambridge University Press:  03 August 2017

Jørgen Christensen-Dalsgaard
Jørgen Christensen-Dalsgaard*
Affiliation:
Astronomisk Institut, Aarhus Universitet, DK-8000 Aarhus C, Denmark

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.

I present evolutionary tracks and curves of constant central hydrogen abundance in diagrams based on frequencies of high-order, low-degree p modes. For stars with masses between 0.7 and 1.5 M⊙, a clean separation is obtained between the effects of varying mass and varying evolutionary state.

Type
Chapter 4: Asteroseismology: Results and Prospects
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 295 - 298
Copyright
Copyright © Reidel 1988 

References

Christensen-Dalsgaard, J., 1982. Mon. Not. R. astr. Soc., 199, 735.Google Scholar
Christensen-Dalsgaard, J., 1984. Space Research Prospects in Stellar Activity and Variability, (ed. Mangeney, A. & Praderie, F., Observatoire de Paris), p. 11.Google Scholar
Gough, D. O., 1986. Highlights in Astronomy, 7, 283.Google Scholar
Scherrer, P. H., Wilcox, J. M., Christensen-Dalsgaard, J. & Gough, D. O., 1983. Solar Phys., 82, 75.Google Scholar
Tassoul, M., 1980. Astrophys. J. Suppl., 43, 469.Google Scholar
Ulrich, R. K., 1986. Astrophys. J., 306, L37.Google Scholar