2008/04/15 by Eliani Ardi, Holger Baumgardt, Shin Mineshige · 1 citation
Physics and Astronomy · #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/589278
25 pages, 9 figures, 3 tables, accepted for publication in ApJ
arxiv created 2008/04/15 · openalex publication_date 2008/07/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
We have investigated the effect of initial mass segregation on the runaway merging of stars. The evolution of multimass, dense star clusters was followed by means of direct N -body simulations of up to 131,072 stars. All clusters started from King models with dimensionless central potentials of 3.0 ⩽ W 0 ⩽ 9.0. Initial mass segregation was realized by varying the minimum mass of a certain fraction of stars whose either (1) distances were closest to the cluster center or (2) total energies were lowest. The second case is more favorable to promote the runaway merging of stars by creating a high-mass core of massive, low-energy stars. Initial mass segregation could decrease the central relaxation time and thus help the formation of a high-mass core. However, we found that initial mass segregation does not help the runaway stellar merger to happen if the overall mass density profile is kept constant. This is due to the fact that the collision rate of stars is not increased due to initial mass segregation. Our simulations show that initial mass segregation is not sufficient to allow runaway merging of stars to occur in clusters with central densities typical for star clusters in the Milky Way.