Revisiting the region of the open cluster NGC 5606

We present polarimetric observations in the UBVRI bands corresponding to 54 stars located in the direction of NGC 5606. Our intention is to analyze the dust characteristics between the Sun and the cluster, as well as to confirm doubtful memberships using Polarimetrie tools. We also want to determine...

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Autores principales: Orsatti, Ana María, Feinstein Baigorri, Carlos, Vega, Ema Irene, Vergne, María Marcela
Formato: Articulo
Lenguaje:Inglés
Publicado: 2007
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/82970
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