PROPER MOTION STUDY OF THE MAGELLANIC CLOUDS USING SPM MATERIAL

Absolute proper motions are determined for stars and galaxies to V = 17.5 over a 450 square degree area that encloses both Magellanic Clouds. The proper motions are based on photographic and CCD observations of the Yale/San Juan Southern Proper Motion program. Multiple, local relative proper motion...

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Détails bibliographiques

Publié dans:	Revista Mexicana de Astronomía y Astrofísica
Auteurs principaux:	K. Vieira, T. Girard, W. van Altena, N. Zacharias, D. Casetti-Dinescu, V. Korchagin, I. Platais, D. Monet, C. López
Format:	Artigo
Langue:	Inglês
Publié:	Universidad Nacional Autónoma de México 2011
Sujets:	Física, Astronomía y Matemáticas
Accès en ligne:	https://www.redalyc.org/articulo.oa?id=57121297046
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