Star cluster formation and disruption time-scales - I. An empirical determination of the disruption time of star clusters in four galaxies
- 1 January 2003
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 338 (3) , 717-732
- https://doi.org/10.1046/j.1365-8711.2003.06083.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 28 references indexed in Scilit:
- Dynamical Evolution of the Mass Function of Globular Star ClustersThe Astrophysical Journal, 2001
- Star Clusters in M33. III. The Youngest PopulationPublications of the Astronomical Society of the Pacific, 1999
- Star Clusters in M33. I. Detection, Morphology, and PhotometryThe Astrophysical Journal Supplement Series, 1999
- Star Clusters in M33. II. Global PropertiesThe Astrophysical Journal, 1999
- Integrated UBV Photometry of 624 Star Clusters and Associations in the Large Magellanic CloudThe Astrophysical Journal Supplement Series, 1996
- Spectral evolution of stellar populations using isochrone synthesisThe Astrophysical Journal, 1993
- Evolution of globular clusters in the GalaxyThe Astrophysical Journal, 1990
- LMC clusters - Age calibration and age distribution revisitedThe Astronomical Journal, 1988
- Age calibration and age distribution for rich star clusters in the Large Magellanic CloudThe Astrophysical Journal, 1985
- Possibility of mass loss in the red-giant stage from H-R diagrams of galactic clustersAstrophysics and Space Science, 1969