The Proper Motion of the Magellanic Clouds. II. New Results for Five Small Magellanic Cloud Fields
We present new results from a ground-based program to determine the proper motion of the Magellanic Clouds (MCs) relative to background quasars (QSOs), being carried out with the Irenee du Pont 2.5 m telescope at Las Campanas Observatory, Chile. The data
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2011 |
| País: | Chile |
| Idioma: | inglés |
| OAI Identifier: | oai:repositorio.anid.cl:10533/240936 |
| Acceso en línea: | https://hdl.handle.net/10533/240936 |
| Access Level: | acceso abierto |
| Sumario: | We present new results from a ground-based program to determine the proper motion of the Magellanic Clouds (MCs) relative to background quasars (QSOs), being carried out with the Irenee du Pont 2.5 m telescope at Las Campanas Observatory, Chile. The data |
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