The Magellanic Clouds as a Template for the Study of Stellar Populations and Galaxy Interactions

Bibcode
2008PASA...25..121C
DOI
10.1071/AS07046
Cioni, M.-R. L.; Bekki, K.; Clementini, G.; de Blok, W. J. G.; Emerson, J. P.; Evans, C. J.; de Grijs, R.; Gibson, B. K.; Girardi, L.; Groenewegen, M. A. T.; Ivanov, V. D.; Leisy, P.; Marconi, M.; Mastropietro, C.; Moore, B.; Naylor, T.; Oliveira, J. M.; Ripepi, V.; van Loon, J. Th.; Wilkinson, M. I.; Wood, P. R.
Referencia bibliográfica

Publications of the Astronomical Society of Australia, Volume 25, Issue 3, pp. 121-128.

Fecha de publicación:
2008
Revista
Publications of the Astronomical Society of Australia
Número de autores
21
Número de autores del IAC
1
Número de citas
14
Número de citas referidas
11
Descripción
The Magellanic System represents one of the best places to study the formation and evolution of galaxies. Photometric surveys of various depths, areas and wavelengths have had a significant impact on our understanding of the system; however, a complete picture is still lacking. VMC (the VISTA near-infrared YJKs survey of the Magellanic System) will provide new data to derive the spatially resolved star formation history and to construct a three-dimensional map of the system. These data combined with those from other ongoing and planned surveys will give us an absolutely unique view of the system opening up the doors to truly new science!
Tipo
Con árbitro
Nubes de Magallanes
Cartografiados

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