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Young open clusters in the Milky Way and Small Magellanic Cloud

Published online by Cambridge University Press:  18 January 2010

C. Martayan
C. Martayan*
Affiliation:
European Organisation for Astronomical Research in the Southern Hemisphere, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago 19, Chile email: cmartaya@eso.org GEPI, Observatoire de Paris, CNRS, Université Paris Diderot, 5 place Jules Janssen, 92195 Meudon Cedex, France
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Abstract

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NGC 6611, Trumpler 14, Trumpler 15, Trumpler 16, and Collinder 232 are very young open clusters located in star-formation regions in the Eagle Nebula and Carina in the Milky Way, and NGC 346 in the Small Magellanic Cloud. With different instrumentation and techniques, it has been possible to detect and classify new Herbig Ae/Be and classical Be stars and to provide new tests/comparisons of the Be stars' appearance models. Special (He-strong) stars in these star-formation regions are also discussed.

Keywords

open clusters and associations: individual (Trumpler 14, Trumpler 15, Trumpler 16, Collinder 232)Magellanic Cloudsgalaxies: star clustersstars: early-typestars: pre–main-sequencestars: emission-lineBestars: evolutiondustextinction
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 466 - 469
Copyright
Copyright © International Astronomical Union 2010

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