Be stars in open clusters in the Small Magellanic Cloud

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dc.creatorMartayan, Christophe
dc.creatorBaade, Dietrich
dc.creatorHubert, Anne-Marie
dc.creatorFloquet, Michele
dc.creatorFabregat, Juan
dc.creatorBertin, Emmanuel
dc.creatorNeiner, Coralie
dc.date2006-09-25
dc.date.accessioned2026-07-07T07:23:21Z
dc.date.available2026-07-07T07:23:21Z
dc.descriptionWe report on the study of the population of B and Be stars in SMC young clusters, performed with the Wide Field Imager in slitless spectroscopic mode at ESO/T2.2m with a filter centered at Halpha. First, we explain the reduction methods we used and our selection of different types of objects. Second, we present results on the proportion of Be stars in SMC clusters, and we compare this proportion to the one observed in the Milky Way. Finally, we also present results on a statistical study of variability of Be stars with OGLE.
dc.descriptionsf2a 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0609678
dc.identifierhttp://arxiv.org/abs/astro-ph/0609678
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/115948
dc.subjectAstrophysics
dc.titleBe stars in open clusters in the Small Magellanic Cloud
dc.typetext

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