Dynamical Processes in Globular Clusters
Stephen L. W. McMillan

TL;DR
This paper reviews the dynamical evolution of globular clusters, highlighting how internal processes lead to dense cores and the formation of exotic objects like blue stragglers through stellar interactions.
Contribution
It provides an overview of the interplay between stellar dynamics and evolution in globular clusters, emphasizing pathways for blue straggler formation.
Findings
Clusters evolve toward high central density
Massive stars and binaries concentrate in cores
Close encounters produce exotic stellar objects
Abstract
Globular clusters are among the most congested stellar systems in the Universe. Internal dynamical evolution drives them toward states of high central density, while simultaneously concentrating the most massive stars and binary systems in their cores. As a result, these clusters are expected to be sites of frequent close encounters and physical collisions between stars and binaries, making them efficient factories for the production of interesting and observable astrophysical exotica. I describe some elements of the competition among stellar dynamics, stellar evolution, and other processes that control globular cluster dynamics, with particular emphasis on pathways that may lead to the formation of blue stragglers.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
