Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-30T00:43:38.384Z Has data issue: false hasContentIssue false

Can stellar mass be measured by asteroseismology?

Published online by Cambridge University Press:  03 August 2017

Roger K. Ulrich*
Affiliation:
Department of Astronomy, University of California, Los Angeles, California 90024

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.

Theoretical calculations show that the detailed pattern of frequencies from stellar oscillations can in principal produce data that can determine stellar masses independent of other input data.

Type
Chapter 4: Asteroseismology: Results and Prospects
Copyright
Copyright © Reidel 1988 

References

Demarque, P., Guenther, D.B., and van Altena, V.F. 1985, Ap. J., 300, 773.Google Scholar
Gelly, B., Grec, G., and Fossat, E. 1986, Astron. and Astroph., 164, 383.Google Scholar
Grec, G., Fossat, E. and Pomerantz, M. 1980, Nature, 288, 541.Google Scholar
Guenther, D.B. and Demarque, P. 1985, Ap. J., 301, 207.Google Scholar
Harvey, J.W. and Duvall, T.L. Jr. 1984, in Solar Seismology from Space (eds. Ulrich, R. K. et al; NASA Jet Propulsion Laboratory Publ. 84-84, Pasadena), p. 165.Google Scholar
Henning, H.M. and Scherrer, P.H. 1986, in Seismology of the Sun and the Distant Stars, (ed. Gough, D.O.; Reidel, Boston), p. 55.CrossRefGoogle Scholar