Binaries in Globular Clusters. A Useful Window: E3.

Details Binaries in Globular Clusters. A Useful Window: E3. Binaries in Globular Clusters. A Useful Window: E3.

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aspc...92..301v&link_type=abstract

Formation of the Galactic Halo...Inside and Out, ASP Conference Series, Vol. 92, 1996, Heather Morrison and Ata Sarajedini, eds.

Computer Science

13

Scientific paper

Deep color magnitude diagrams of the loose globular cluster E3 are presented. The high-precision photometric measurements show a clear-cut secondary sequence of stars which runs parallel to the main sequence (MS) and is interpreted as composed of binary systems. A preliminary analysis of the radial distribution of binary candidates in the cluster shows that they have a more centrally concentrated distribution than single MS-stars in the inner two core radii from the cluster center. Accurate analysis of the data will provide the first large sample (N > 100) of binary candidates in globular clusters.

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