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Can stellar mass be measured by asteroseismology?
Published online by Cambridge University Press: 03 August 2017
Abstract
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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
- Information
- Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 299 - 302
- Copyright
- Copyright © Reidel 1988
References
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
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