期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 419, 期 2, 页码 1350-1361出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2011.19791.x
关键词
stars: abundances; Galaxy: abundances; open clusters and associations: individual: NGC 752; open clusters and associations: individual: NGC 1817; open clusters and associations: individual: NGC 2360; open clusters and associations: individual: NGC 2506
资金
- Robert A. Welch Foundation of Houston, Texas [F-634]
We have analysed high-dispersion echelle spectra (R greater than or similar to 50 000) of red giant members for four open clusters to derive abundances for many elements. The spread in temperatures and gravities being very small among the red giants nearly the same stellar lines were employed thereby reducing the random errors. The errors of average abundance for the cluster were generally in the range 0.02-0.07 dex. Our present sample covers Galactocentric distances of 8.3-10.5 kpc. The [Fe/H] values are -0.02 +/- 0.05 for NGC 752, -0.07 +/- 0.06 for NGC 2360, -0.11 +/- 0.05 for NGC 1817 and -0.19 +/- 0.06 for NGC 2506. Abundances relative to Fe for elements from Na to Eu are equal within measurement uncertainties to published abundances for thin-disc giants in the field. This supports the view that field stars come from disrupted open clusters.
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