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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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , , , , , , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2011
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57121297046 |
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