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Clusters in Extragalactic HII Regions and their Modelling

Published online by Cambridge University Press:  03 August 2017

Rosa María González Delgado
Rosa María González Delgado*
Affiliation:
Instituto de Astrofísica de Andalucía (CSIC). Apdo. 3004, 18080 Granada, Spain

Abstract

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This review deals with properties of very young (≤ 10–20 Myr) stellar clusters which are in the nebular phase and are embedded in photoionized regions (classical extragalactic HII regions (RHIIs) or starburst galaxies). Based on the analysis of the integrated light of these clusters at the UV and optical wavelengths, different techniques are discussed that allow to estimate in consistent the stellar content and the evolutionary state of the ionizing clusters. Figures illustrating this contribution can be found in: http://www.iaa.csic.es/∼rosa/

Type
Part 3. Super Star Clusters and Associations
Information
Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 428 - 438
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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