Open AccessDirect N ‐body modelling of stellar populations: blue stragglers in M67
Author(s) -
Hurley Jarrod R.,
Tout Christopher A.,
Aarseth Sverre J.,
Pols Onno R.
Publication year - 2001
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2001.04220.x
Subject(s) - physics , blue straggler , astrophysics , stellar collision , mass segregation , stellar mass , astronomy , open cluster , globular cluster , stellar evolution , stars , star formation
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.