Explaining the mass-to-light ratios of globular clusters

Astronomy and Astrophysics

Volumn 486, Issue 3, 2008, Pages

  Kruijssen, J M D ^a,b  

^a UTRECHT UNIVERSITY   (Netherlands)

^b LEIDEN UNIVERSITY   (Netherlands)

Author keywords

Galaxies: star clusters; Galaxies: stellar content; Galaxy: globular clusters: general; Methods: analytical

Indexed keywords

GALAXIES; ION BEAMS; METALLIZING; STARS;

CLUSTER MASS; CLUSTER MODELLING; DYNAMICAL EFFECTS; ENERGY EQUIPARTITION; EVOLUTION (CO); GLOBULAR CLUSTERS; LOW-MASS STARS; METALLICITIES; METALLICITY; MILKY WAY; STELLAR EVOLUTIONS; TIME SCALING; TIME-SCALES;

DISSOLUTION;

EID: 47749151812     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810237     Document Type: Article

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