Massive infrared clusters in the milky way

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dc.contributor.authorChené, André-Nicolas
dc.contributor.authorRamírez Alegría, Sebastián
dc.contributor.authorBorissova, Jordanka
dc.contributor.authorHervé, Anthony
dc.contributor.authorMartins, Fabrice
dc.contributor.authorKuhn, Michael
dc.contributor.authorMinniti, Dante
dc.date.accessioned2023-08-29T14:32:06Z
dc.date.available2023-08-29T14:32:06Z
dc.date.issued2016-11
dc.descriptionIndexación: Scopus.es
dc.description.abstractOur position in the Milky Way (MW) is both a blessing and a curse. We are nearby to many star clusters, but the dust that is a product of their very existence obscures them. Also, many massive young clusters are expected to be located near, or across the Galactic Center, where the dust extinction is extreme (AV > 15 mag) and can be better penetrated by infrared photons. This paper reviews the discoveries and the study of new MW massive stars and massive clusters made possible by near infrared observations that are part of the VISTA Variables in the V´ıa L´actea (VVV) survey. It discusses what the studies of their fundamental parameters have taught us.es
dc.description.urihttps://www-cambridge-org.recursosbiblioteca.unab.cl/core/journals/proceedings-of-the-international-astronomical-union/article/massive-infrared-clusters-in-the-milky-way/4618C586D375CF6772CD731EA7802195
dc.identifier.citationProceedings of the International Astronomical Union. Open Access. Volume 12, Issue S329, Pages 263 - 270. 1 November 2016es
dc.identifier.doi10.1017/S1743921317002988
dc.identifier.issn1743-9213
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/52884
dc.language.isoenes
dc.publisherCambridge University Presses
dc.subjectSurveyses
dc.subjectStars: Distanceses
dc.subjectStars: Evolutiones
dc.subjectStars: Fundamental Parameterses
dc.subjectStars: Wolf-Rayetes
dc.subject(Galaxy:) Open Clusters and Associations: Generales
dc.titleMassive infrared clusters in the milky wayes
dc.typeArtículoes
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