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Sur La Masse D’une Binaire Spectroscopique Membre D’une Etoile Double Visuelle

Published online by Cambridge University Press:  12 April 2016

P. Couteau
P. Couteau*
Affiliation:
Observatoire de Nice

Abstract

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We describe a method which interposes a relation Mass-Luminosity in order to calculate the dynamic parallax and the masses of the components in a system of known orbit which involves a spectroscopic binary. We apply the method to a few cases.

Resumen

Resumen

Se describe un método, que interpone una relación masa-luminosidad para calcular la paralaje dinámica y las masas de las componentes de un sistema visual de órbita conocida, cuando una de aquellas es una binaria espectroscópica. Se aplica el método a algunos casos específicos.

Type
Session 3
Information
International Astronomical Union Colloquium , Volume 33: Observational Parameters and Dynamical Evolution of Multiple Stars , May 1977 , pp. 77 - 83
Copyright
Copyright © Otto G. Franz and Paris Pismis 1977

References

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