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The IMF and Mass Segregation in Young Galactic Starburst Clusters

  • Eva K. Grebel
Part of the Astrophysics and Space Science Library book series (ASSL, volume 327)

Abstract

The pronounced mass segregation in very young rich Galactic starburst clusters like NGC 3603 and Arches may be due to their extremely short relaxation times and high densities, which appear to lead to rapid dissolution. To what extent mass segregation in these systems is primordial as opposed to evolutionary cannot easily be distinguished. While flat in their centers, the total mass functions of these rich clusters seem close to a Salpeter slope, supporting a universal IMF.

Keywords

Mass Function Massive Star Galactic Center Hubble Space Telescope Star Cluster 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer 2005

Authors and Affiliations

  • Eva K. Grebel
    • 1
  1. 1.Astronomical Institute of the University of BaselSwitzerland

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