Hostname: page-component-7479d7b7d-m9pkr Total loading time: 0 Render date: 2024-07-12T01:22:00.599Z Has data issue: false hasContentIssue false
  • English
  • Français

The Size Distribution of Massive Young Clusters

Published online by Cambridge University Press:  03 August 2017

Jesús Maíz-Apellániz
Jesús Maíz-Apellániz*
Affiliation:
STSc!, 3700 San Martin Drive, Baltimore, MD 21218, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have searched the WFPC2/HST archive for data on nearby massive young clusters with low extinction and we have analyzed 27 such objects. A clear dichotomy between objects with a compact core and without it is observed. We attribute this bimodality to the initial conditions of the parent giant molecular clouds and we discuss its implication towards the long-term evolution of the clusters.

Type
Part 4. Star Cluster Formation and Evolution: Theory and Observation
Information
Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 697 - 699
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

Fall, S. M. 2002, these proceedings Google Scholar
Ho, L. C. & Filippenko, A. V. 1996, ApJ, 472, 600 Google Scholar
Maíz-Apellániz, J. 2001, submitted to ApJ Google Scholar
Walborn, N. R. & Parker, J. Wm. 1992, ApJ, 399, L87 CrossRefGoogle Scholar
Wiseman, J. J. & Ho, P. T. P. 1998, ApJ, 502, 676 Google Scholar