NGC 2354: a moderately metal-poor open cluster in Canis Major

New UBV, DDO and CMT₁T₂ photometric data of stars in NGC 2354 demonstrate that the duster red giant branch is consistent with that predicted by models with mass loss and moderate overshooting. The cluster metallicity ([Fe/H] = -0.33 ± 0.07) is compatible with the existence of a chemical composition...

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Guardado en:
Detalles Bibliográficos
Autores principales: Clariá, J.J., Piatti, A.E.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1994
Materias:
Astronomía
Galaxia
ngc 2354
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/159802
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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