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Modeling Eclipsing Binaries in Globular Clusters

Published online by Cambridge University Press:  22 February 2018

E.F. Milone
Affiliation:
RAO, University of Calgary, Calgary, AB, Canada
J. Kallrath
Affiliation:
BASF, Ludwigshafen, Germany Dept. of Astronomy, University of Florida, Gainesville, FL, USA
C.R. Stagg
Affiliation:
RAO, University of Calgary, Calgary, AB, Canada Joliet Junior College, Joliet, IL, USA
M.D. Williams
Affiliation:
RAO, University of Calgary, Calgary, AB, Canada

Abstract

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We describe the use of eclipsing binaries to derive fundamental properties of the binary star components in a cluster. The method requires the use of reliable isochrones and accurate properties of stars that lie along them.

Resumen

Resumen

Describimos el uso de las binarias eclipsantes para derivar propiedades fundamentales de las componentes de las binarias en cúmulos estelares. El método requiere el uso de isocronas confiables y de propiedades exactas de las estrellas situadas en éstas.

Type
Observational Results for Very Young Binaries
Copyright
Copyright © Instituto de Astronomia – Mexico 2004

References

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