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Modeling Eclipsing Binaries in Globular Clusters

Published online by Cambridge University Press:  22 February 2018

E.F. Milone,
J. Kallrath,
C.R. Stagg and
M.D. Williams
E.F. Milone
Affiliation:
RAO, University of Calgary, Calgary, AB, Canada
J. Kallrath
Affiliation:
BASF, Ludwigshafen, GermanyDept. of Astronomy, University of Florida, Gainesville, FL, USA
C.R. Stagg
Affiliation:
RAO, University of Calgary, Calgary, AB, CanadaJoliet 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.

Keywords

BinariesEclipsing — GalaxiesClusters — StarsFundamental Data

Information

Type
Observational Results for Very Young Binaries
Information
International Astronomical Union Colloquium , Volume 191: The Environment and Evolution of Double and Multiple Stars , August 2004, pp. 109 - 115
Copyright
Copyright © Instituto de Astronomia – Mexico 2004

References

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