Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-12-05
Mon.Not.Roy.Astron.Soc. 323 (2001) 630
Astronomy and Astrophysics
Astrophysics
26 pages, 18 figures, accepted for publication in MNRAS
Scientific paper
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 = 10000 simulations in order to quantify the rate of escape of stars from a cluster subject to the Galactic tidal field.
Aarseth Sverre J.
Hurley Jarrod R.
Pols Onno R.
Tout Christopher A.
No associations
LandOfFree
Direct N-body Modelling of Stellar Populations: Blue Stragglers in M67 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 Direct N-body Modelling of Stellar Populations: Blue Stragglers in M67, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct N-body Modelling of Stellar Populations: Blue Stragglers in M67 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-30755