Initial conditions of formation of starburst clusters: constraints from stellar dynamics

TL;DR

This paper investigates the formation of starburst clusters by examining stellar dynamics, emphasizing the roles of cluster expansion, hierarchical merging, and gas expulsion in shaping observed young massive clusters.

Contribution

It provides new insights into the initial conditions of starburst cluster formation, highlighting the importance of residual gas expulsion regardless of formation mode.

Findings

Residual gas expulsion is essential for cluster shaping.

Hierarchical merging influences cluster properties.

Secular expansion impacts cluster evolution.

Abstract

How starburst clusters form out of molecular clouds is still an open question. In this article, I highlight some of the key constraints in this regard, that one can get from the dynamical evolutionary properties of dense stellar systems. I particularly focus on secular expansion of massive star clusters and hierarchical merging of sub-clusters, and discuss their implications vis-a-vis the observed properties of young massive clusters. The analysis suggests that residual gas expulsion is necessary for shaping these clusters as we see them today, irrespective of their monolithic or hierarchical mode of formation.