Photometry of Fourteen Main Belt Asteroids
The results of CCD photometry of 14 main belt asteroids obtained between1996 and 2000 are presented. For most of them, the V or R composite lightcurvesand the values of the synodic rotational period are derived. There exists no previousdetermination of the period for 11 of the observed objects.
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2003
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57139106 |
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