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Realistic models for evolving globular clusters: core collapse with a mass spectrum
Author(s) -
B. W. Murphy,
H. N. Cohn
Publication year - 1988
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/232.4.835
Subject(s) - physics , globular cluster , astrophysics , surface brightness , stars , mass segregation , initial mass function , velocity dispersion , stellar mass , power law , star cluster , stellar density , star formation , luminosity , cluster (spacecraft) , astronomy , galaxy , statistics , mathematics , computer science , programming language

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