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The Top-Heavy Mass Function of the Young Super Star Cluster M82-F
Published online by Cambridge University Press: 03 August 2017
Abstract
We derive a dynamical mass of 1.2 ± 0.1 × 106 M⊙ for the young SSC M82-F and determine that the current (LV/M)⊙ is a factor of ∼ 5 higher than that predicted by a standard Kroupa (2001) IMF. This suggests that M82-F has a deficit of low mass stars and will not survive to become an old globular cluster.
- Type
- Part 3. Super Star Clusters and Associations
- Information
- Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 479 - 482
- Copyright
- Copyright © Astronomical Society of the Pacific 2002