期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 391, 期 3, 页码 1482-1488出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2008.14011.x
关键词
stars: abundances; open clusters and associations: individual: Trumpler 20
资金
- National Science Foundation [AST 04-06689]
- W. M. Keck Foundation
- Gordon and Betty Moore Foundation
- Chilean Centro de Astrofisica FONDAP [15010003]
- Fundacao para Ciencia e a Tecnologia (Portugal) [SFRH/BD/21502/2005]
- Fundação para a Ciência e a Tecnologia [SFRH/BD/21502/2005] Funding Source: FCT
We show that the open cluster Trumpler 20, contrary to the earlier findings, is actually an old Galactic open cluster. New CCD photometry and high-resolution spectroscopy are used to derive the main parameters of this cluster. At [Fe/H] = -0.11 for a single red giant star, the metallicity is slightly subsolar. The best fit to the colour-magnitude diagrams is achieved using a 1.3-Gyr isochrone with convective overshoot. The cluster appears to have a significant reddening at E(B-V) = 0.46 (for B0 spectral type), although for red giants this high reddening yields the colour temperature exceeding the spectroscopic T-eff by about 200 K. Trumpler 20 is a very rich open cluster, containing at least 700 members brighter than M-V = +4. It may extend over the field of view available in our study at 20 x 20 arcmin(2).
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