Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 323, Issue 3, Pages 630-650Publisher
BLACKWELL SCIENCE LTD
DOI: 10.1046/j.1365-8711.2001.04220.x
Keywords
methods : N-body simulations; binaries : general; blue stragglers; stars : evolution; globular clusters : general; open clusters and associations : individual : M67
Categories
Ask authors/readers for more resources
We present a state-of-the-art N-body code which includes a detailed treatment of stellar and binary evolution as well as the cluster dynamics. This code is ideal for investigating all aspects relating to the evolution of star clusters and their stellar populations. It is applicable to open and globular clusters of any age. We use the N-body code to model the blue straggler population of the old open cluster M67. Preliminary calculations with our binary population synthesis code show that binary evolution alone cannot explain the observed numbers or properties of the blue stragglers. On the other hand, our N-body model of M67 generates the required number of blue stragglers and provides formation paths for all the various types found in M67. This demonstrates the effectiveness of the cluster environment in modifying the nature of the stars it contains, and highlights the importance of combining dynamics with stellar evolution. We also perform a series of N = 10 000 simulations in order to quantify the rate of escape of stars from a cluster subject to the Galactic tidal field.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available