The photometric evolution of dissolving star clusters II. Realistic models. Colours and M/L ratios

Astronomy and Astrophysics

Volumn 502, Issue 3, 2009, Pages 817-832

  Anders, P ^a   Lamers, H J G L M ^a   Baumgardt, H ^b  

^a UTRECHT UNIVERSITY   (Netherlands)

^b UNIVERSITY OF BONN   (Germany)

Author keywords

Galaxies: Star clusters, methods: Data analysis; Galaxy: Globular clusters: General; Galaxy: Open clusters and associations: General

Indexed keywords

AGE DETERMINATION; AGE DIFFERENCES; COMPACT OBJECTS; DARK MATTER; DISRUPTION TIME; DYNAMICAL SIMULATION; GALAXIES: STAR CLUSTERS, METHODS: DATA ANALYSIS; GALAXY: GLOBULAR CLUSTERS: GENERAL; GALAXY: OPEN CLUSTERS AND ASSOCIATIONS: GENERAL; HIGH-MASS STARS; LOW-MASS STARS; MASS FUNCTIONS; METALLICITIES; MODEL RESULTS; N-BODY SIMULATION; PARAMETRISATION; PHYSICAL PARAMETERS; REALISTIC MODEL; SIMPLIFYING ASSUMPTIONS; STANDARD MODEL; STAR CLUSTERS; STELLAR EVOLUTIONS; STELLAR MASS; STELLAR POPULATIONS; SYNTHESIS CODE; SYNTHESIS MODELS;

DISSOLUTION; GALAXIES; PHOTOMETRY; STARS;

SIMULATORS;

EID: 68649107596     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810615     Document Type: Article

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