Clusters in extragalactic HII regions and their modelling

dc.creatorDelgado, Rosa M. Gonzalez
dc.date2001-06-18
dc.date.accessioned2026-07-07T01:58:57Z
dc.date.available2026-07-07T01:58:57Z
dc.descriptionThis 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.
dc.descriptionReview to appear in "Extragalactic Star Clusters", eds. E.W. Grebel, D. Geisler, D. Minniti, IAU Symp. Series PASP 207. Related figures can be found at: http://www.iaa.csic.es/~rosa/
dc.identifierhttps://arxiv.org/abs/astro-ph/0106297
dc.identifierhttp://arxiv.org/abs/astro-ph/0106297
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2918
dc.subjectAstrophysics
dc.titleClusters in extragalactic HII regions and their modelling
dc.typetext

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