Photometric and kinematic study of the Galactic open cluster NGC 2309
We have obtained CCD UBVIKC photometry for NGC 2309, a relatively poor open cluster (OC) projected onto a rich star field in Monoceros. Probable cluster members have been identified for the first time from sound photometric criteria. We have derived the angular radius and the fundamental cluster par...
| Autores: | , , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2010 |
| País: | Argentina |
| Recursos: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repositorio: | CONICET Digital (CONICET) |
| Idioma: | inglés |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/19164 |
| Acesso em linha: | http://hdl.handle.net/11336/19164 |
| Access Level: | acceso abierto |
| Palavra-chave: | CLUSTERS PHOTOMETRY https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| Resumo: | We have obtained CCD UBVIKC photometry for NGC 2309, a relatively poor open cluster (OC) projected onto a rich star field in Monoceros. Probable cluster members have been identified for the first time from sound photometric criteria. We have derived the angular radius and the fundamental cluster parameters. The resulting reddening and distance values place this object among the relatively most reddened and distant known OCs projected towards the direction of NGC 2309. A detailed version of this work can be seen in PASP, 122, 288 (2010). |
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