Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-12-18
Astronomy and Astrophysics
Astrophysics
4 pages, ApJ style, 2 figures, 2 tables, ApJL submitted
Scientific paper
We study the evolution of binary stars in globular clusters using a novel approach combining a state-of-the-art population synthesis code with a simple treatment of dynamical interactions in the dense cluster core. We find that the combination of stellar evolution and dynamical interactions (binary-single and binary-binary) leads to a rapid depletion of the binary population in the cluster core. The maximum binary fraction today in the core of a typical dense cluster like 47 Tuc, assuming an initial binary fraction of 100%, is only about 5%. We show that this is in good agreement with recent HST observations of close binaries in the core of 47 Tuc, provided that a realistic distribution of binary periods is used to interpret the results. Our findings also have important consequences for the dynamical modeling of globular clusters, suggesting that ``realistic models'' should incorporate much larger initial binary fractions than has usually been done in the past.
Belczynski Krzysztof
Fregeau John M.
Ivanova Natalia
Rasio Frederic A.
No associations
LandOfFree
On the Maximum Binary Fraction in Globular Cluster Cores does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On the Maximum Binary Fraction in Globular Cluster Cores, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Maximum Binary Fraction in Globular Cluster Cores will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-307507