In:
Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 174 ( 1996), p. 397-398
Abstract:
We examine two globular cluster formation scenarios with SPH simulations, using GRAPE-3AF. First model is the spontaneous collapse, which is found to induce a disruption of the system. However, the system can survive when sufficiently high external pressure exists. Second model is the collision of the two proto-cluster clouds, which can form a bound stellar system due to efficient cooling and a burst of star formation.
Type of Medium:
Online Resource
ISSN:
0074-1809
DOI:
10.1017/S007418090000200X
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1996
SSG:
16,12
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