The apparent overdensity of open clusters in the Canis Major overdensity

The exciting debate on the existence and nature of the relatively recent discovery of the so-called Canis Major (CMa) overdensity is re-examined here based on the positions, reddenings, ages and metallicities of Galactic open clusters (OCs). The data used to carry out the current study were taken fr...

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Detalles Bibliográficos
Publicado:	2008
Materias:	Galaxies: dwarf Galaxy: structure Open clusters and associations: general
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17453933_v390_n1_pL54_Piatti http://hdl.handle.net/20.500.12110/paper_17453933_v390_n1_pL54_Piatti
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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