V588 Mon and V589 Mon, Two Delta Scuti Stars in the Direction of NGC 2264
Both differential and absolute photoelectric photometry of the short periodvariable stars V588 Mon (W2) and V589 Mon (W20) in the direction of the OpenCluster NGC2264 has been carried out. From uvbyB photoelectric photometry,the distances and physical characteristics of each star have been estimated...
| Autores: | , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2002 |
| País: | México |
| Institución: | Universidad Nacional Autónoma de México |
| Repositorio: | Redalyc-UNAM |
| OAI Identifier: | oai:redalyc.org:57138104 |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57138104 |
| Access Level: | acceso abierto |
| Palabra clave: | Física, Astronomía y Matemáticas V589 MON) DELTA SCUTI STARS: INDIVIDUAL (V588 MON |
| Sumario: | Both differential and absolute photoelectric photometry of the short periodvariable stars V588 Mon (W2) and V589 Mon (W20) in the direction of the OpenCluster NGC2264 has been carried out. From uvbyB photoelectric photometry,the distances and physical characteristics of each star have been estimated and arepresented. The differential photometry of the variables allowed us to carry out aFourier analysis of the data. The frequencies determined for each star are: for W2,7.1865 c/d and for W20, 7.4385 c/d. The issue of cluster membership is discussed. |
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