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The Stellar Luminosity Function and Binary Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
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If all stars within a small volume surrounding the sun are counted we obtain an approximation of the low-mass single-star luminosity function. Alternatively, deep photographic surveys cannot resolve most of the binary systems, and consequently we obtain an approximation to the system luminosity function. Comparing the single-star and system luminosity functions we derive the stellar mass function and constrain the properties of binary systems.
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- Copyright © Astronomical Society of the Pacific 1992
References
Wielen, R., Jahreiss, H., & Krüger, R., 1983, In The Stare and Stellar Luminosity Function IAU Coll. 76, eds. Philip, A.G. Davis and Upgren, A.R. (Schenectady: L. Davis Press), p. 163
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