Surviving gas expulsion with substructure
Author(s) -
Paweł L. Lee,
S. P. Goodwin
Publication year - 2016
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/stw988
Subject(s) - substructure , physics , astrophysics , cluster (spacecraft) , virial theorem , galaxy , structural engineering , computer science , engineering , programming language
We investigate the reaction of clumpy stellar distributions to gas expulsion. We show that regions containing highly unbound substructures/subclusters after gas expulsion can produce a significant final bound cluster. The key quantity in determining if a region is able to form a bound cluster is the global virial ratio, and so regions must be looked at as a whole rather than by individual substructure/subclusters when determining if they might survive as a bound cluster.
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