Why simple stellar population models do not reproduce the colours of Galactic open clusters

Astronomy and Astrophysics

Volumn 507, Issue 1, 2009, Pages

  Piskunov, A E ^a,b,c   Kharchenko, N V ^a,c,d   Schilbach, E ^c   Roser S ^c   Scholz, R D ^a   Zinnecker, H ^a  

^a ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^b INSTITUTE OF ASTRONOMY   (Russian Federation)

^c ASTRONOMISCHES RECHEN INSTITUT   (Germany)

^d NATIONAL ACADEMY OF SCIENCES OF UKRAINE   (Ukraine)

Author keywords

Galaxies: fundamental parameters; Galaxies: photometry; Galaxies: star clusters; Galaxies: starburst; Galaxy: stellar content; Open clusters and associations: general

Indexed keywords

CLUSTER MASS; FUNDAMENTAL PARAMETERS; GALAXIES: FUNDAMENTAL PARAMETERS; GALAXIES: PHOTOMETRY; GALAXIES: STAR CLUSTERS - GALAXIES; INITIAL MASS; MASS DISTRIBUTION; MASS FUNCTIONS; MODEL FIT; MONTE CARLO SIMULATION; OPEN CLUSTERS; OPEN CLUSTERS AND ASSOCIATIONS: GENERAL; STELLAR POPULATIONS;

COLOR; MONTE CARLO METHODS; PHOTOMETERS; PHOTOMETRY; SIMULATORS;

GALAXIES;

EID: 70449645517     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913270     Document Type: Article

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