A revision of the fundamental parameters of the open cluster Hogg 15 and the projected star WR 47

We revise the fundamental parameters of the faint open cluster Hogg 15, for which two recent colour-magnitude diagram (CMD) studies have obtained significantly different ages. In the present study, we combine a series of methods trying to constrain age, together with other fundamental parameters. We...

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Detalles Bibliográficos
Autores principales: Piatti, A.E., Bica, E., Santos Jr., J.F.C., Clariá, J.J.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v387_n1_p108_Piatti
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