Direct N-body modelling of stellar populations: blue stragglers in M67

We present a state-of-the-art N-body code which includes a detailed treatme nt of stellar and binary evolution as well as the cluster dynamics. This co de is ideal for investigating all aspects relating to the evolution of star clusters and their stellar populations. It is applicable to open and globu lar 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 ex plain the observed numbers or properties of the blue stragglers. On the oth er hand, our N-body model of M67 generates the required number of blue stra gglers and provides formation paths for all the various types found in M67. This demonstrates the effectiveness of the cluster environment in modifyin g the nature of the stars it contains, and highlights the importance of com bining 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 clu ster subject to the Galactic tidal field.