Eugene F. Milone, Josef Kallrath, C. R. Stagg, Matthew D. Williams
Abstract
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Abstract 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.
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Abstract 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.
Key concepts: Globular cluster, Binary number, Astrophysics, Stars, Physics, Binary star, Cluster (spacecraft), Star cluster