PROPER MOTION OF THE MAGELLANIC CLOUDS USING SPM
Absolute proper motions are determined for stars and galaxies to V = 17 . 5 over a 450 square-degree area that includes the Magellanic Clouds, using photographic and CCD observations of the Yale/ San Juan Southern Proper Motion program. Multiple, local relative proper motion measures w ere combined...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , , , , , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2014
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57131045014 |
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