Luminosity and mass functions of galactic open clusters II: NGC 4852

We present wide-field deep UBVI photometry for the previously unstudied open cluster NGC 4852 down to a limiting magnitude I ∼ 24, obtained from observations taken with the Wide Field Imager camera on-board the MPG/ESO 2.2 m telescope at La Silla (ESO, Chile). These data are used to obtain the first...

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Detalles Bibliográficos
Autores principales:	Carraro, G., Baume, Gustavo, Piotto, G., Méndez, R. A., Schmidtobreik, L.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2005
Materias:	Ciencias Astronómicas C-M diagrams Hertzsprung-Russell (HR) Open clusters and associations: individual: NGC 4852
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/83279
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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