Massive infrared clusters in the Milky Way

André Nicolas Chené, Sebastian Ramírez Alegría, Jordanka Borissova, Anthony Hervé, Fabrice Martins, Michael Kuhn, Dante Minniti

Resultado de la investigación: Contribución a una revistaArtículo

Resumen

Our 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 (A V > 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 Vía Láctea (VVV) survey. It discusses what the studies of their fundamental parameters have taught us.

Idioma originalInglés
Páginas (desde-hasta)263-270
Número de páginas8
PublicaciónProceedings of the International Astronomical Union
Volumen12
N.ºS329
DOI
EstadoPublicada - 1 nov 2016

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica
  • Ciencias planetarias y espacial

Huella Profundice en los temas de investigación de 'Massive infrared clusters in the Milky Way'. En conjunto forman una huella única.

  • Citar esto

    Chené, A. N., Ramírez Alegría, S., Borissova, J., Hervé, A., Martins, F., Kuhn, M., & Minniti, D. (2016). Massive infrared clusters in the Milky Way. Proceedings of the International Astronomical Union, 12(S329), 263-270. https://doi.org/10.1017/S1743921317002988