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Cambridge University Press (CUP), Publications of the Astronomical Society of Australia, 3(25), p. 121-128, 2008

DOI: 10.1071/as07046

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

Journal article published in 2008 by M.-R. L. Cioni, K. Bekki ORCID, G. Clementini ORCID, W. J. G. de Blok, J. P. Emerson, C. J. Evans, R. de Grijs ORCID, B. K. Gibson ORCID, L. Girardi, M. A. T. Groenewegen, V. D. Ivanov ORCID, P. Leisy, M. Marconi ORCID, C. Mastropietro, B. Moore and other authors.
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractThe 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!

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