The fate of the pre-main sequence-rich clusters Collinder 197 and vdB92: Dissolution?

Astronomy and Astrophysics

Volumn 516, Issue 25, 2010, Pages

  Bonattol, C ^a   Bica, E ^a  

^a FEDERAL UNIVERSITY OF RIO GRANDE DO SUL   (Brazil)

Author keywords

open clusters and associations: general; open clusters and associations: individual: Collinder 197; open clusters and associations: individual: vdB 92

Indexed keywords

CHROMIUM; DISPERSIONS; PHOTOMETRY; STARS;

COLOUR-MAGNITUDE DIAGRAMS; DYNAMICAL EFFECTS; DYNAMICAL EQUILIBRIUM; EMBEDDED CLUSTERS; GALACTIC STARS; MOLECULAR CLOUDS; NEAR-INFRARED PHOTOMETRY; OPEN CLUSTERS AND ASSOCIATIONS: GENERAL; OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: VDB 92; OPEN CLUSTERS AND ASSOCIATIONS:INDIVIDUAL; PMS STARS; PRE-MAIN SEQUENCES; PROPER MOTION; RADIAL DENSITY DISTRIBUTION; STAR CLUSTERS; STAR FORMATIONS; STAR-FORMATION PROCESS; STELLAR MASS; VELOCITY DISPERSION;

DISSOLUTION;

EID: 77957593439     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014146     Document Type: Article

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