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The Environments of the Massive Star Clusters in the Carina Nebula
Published online by Cambridge University Press: 03 August 2017
Abstract
We have imaged over an extensive field the 3.29-μm emission from the Carina Nebula. This emission arises from polycyclic aromatic hydrocarbons which are excellent tracers of photodissociation regions. The results emphasis the two very different environments of the massive star clusters of the nebula, Trumpler 14 and 16.
- Type
- Part 1. The Star Clusters of Local Group Galaxies
- Information
- Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 129 - 131
- Copyright
- Copyright © Astronomical Society of the Pacific 2002