Clustered Star Formation: A Review
arXiv:1208.0011 · doi:10.1007/978-3-319-03041-8_86
Abstract
In this contribution I present a review of star formation in clusters. I begin by discussing the various definitions of what constitutes a star cluster, and then compare the outcome of star formation (IMF, multiplicity, mass segregation and structure and morphology) in different star-forming regions. I also review recent numerical models of star formation in clusters, before ending with a summary of the potential effects of dynamical evolution in star clusters.
6 pages, invited review to appear in the proceedings of 'The Labyrinth of Star Formation', Crete, 18-22 June 2012
References in corpus (8)
- A Spitzer Survey of Young Stellar Clusters within One Kiloparsec of the Sun: Cluster Core Extraction and Basic Structural Analysis
- Stellar, brown dwarf and multiple star properties from a radiation hydrodynamical simulation of star cluster formation
- Dynamical mass segregation on a very short timescale
- Using the minimum spanning tree to trace mass segregation
- The distinction between star clusters and associations
- The effects of dynamical interactions on planets in young substructured star clusters
- Testing the universality of star formation - I. Multiplicity in nearby star-forming regions
- The evolution of binary populations in cool, clumpy star clusters