Collisional Formation of Very Massive Stars in Young Dense Clusters

Details Collisional Formation of Very Massive Stars in Young Dense Clusters Collisional Formation of Very Massive Stars in Young Dense Clusters

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21741604m&link_type=abstract

American Astronomical Society, AAS Meeting #217, #416.04; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Numerical studies of the early evolution of star clusters have traditionally been based on full hydrodynamic treatments or a purely gravitational N-body approach . I will
discuss recent work that pushes the N-body techniques toward a more realistic gas treatment. In particular I will focus on the behavior of very young clusters as they accrete gas, leading to compact configurations that are robust to gas expulsion, and in extreme cases to the collisional growth of very massive stars.

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