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Masses, Radii and Luminosities from Analysis of Eclipsing Binaries
Published online by Cambridge University Press: 04 August 2017
Abstract
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The reliability of values of the fundamental properties of stars derived from eclipsing binary analysis is discussed in terms of general concepts. Since the principles involved in the determination of masses and radii are simple, the heart of the matter is the care and judgment with which the relevant spectrographic and photometric observations are obtained and analyzed. Problems in the evaluation of the radiative properties require special attention.
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- 1. Review Papers
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- Copyright © Reidel 1985
References
This reference contains citations of many spectrographic and photometric investigations of numerous authors.Google Scholar
Papers on spectrographic problems, not cited in the text.Google Scholar
Popper, D.M.
1966, Trans. IAU Vol. X11B, ed. Pecker, J.-C., (Academic Press: New York) p. 485.Google Scholar
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Popper, D.M.
1970, in IAU Colloquium No. 6, Mass Loss and Evolution in Close Binaries, eds. Gyldenkerne, K. and West, R.M. (Copenhagen U. Publ. Fund: Copenhagen), p. 13.Google Scholar
Papers on light curve analysis, not cited in the text.Google Scholar
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