The ACS Survey of Galactic Globular Clusters - XII. Photometric Binaries along the Main Sequence

Authors

A. P. Milone, University of La Laguna
G. Piotto, University of Padua
L. R. Bedin, INAF-Astronomical Observatory of PaduaFollow
A. Aparicio, University of La LagunaFollow
J Anderson, Space Telescope Science InstituteFollow
A Sarajedini, University of Florida
A. F. Marino, Max Plank Institute for Astrophysics
A. Moretti, INAF-Astronomical Observatory of Padua
M. B. Davies, Lund Observatory
B. Chaboyer, Dartmouth CollegeFollow

Document Type

Article

Publication Date

1-1-2012

Publication Title

Astronomy and Astrophysics

Abstract

The fraction of binary stars is an important ingredient to interpret globular cluster dynamical evolution and their stellar population.

DOI

10.1051/0004-6361/201016384

Dartmouth Digital Commons Citation

Milone, A. P.; Piotto, G.; Bedin, L. R.; Aparicio, A.; Anderson, J; Sarajedini, A; Marino, A. F.; Moretti, A.; Davies, M. B.; and Chaboyer, B., "The ACS Survey of Galactic Globular Clusters - XII. Photometric Binaries along the Main Sequence" (2012). Dartmouth Scholarship. 526.
https://digitalcommons.dartmouth.edu/facoa/526