Metallicity distribution of F-dwarf stars in the solar neighbourhood
Tóm tắt
A volume-limited sample of F-dwarfs is chosen from Knude (1989) with low radial velocity as well as distance from the sun and compared with the expected model metallicity [Fe/H] distributions, taking the possible chemical inhomogeneity into account. There is found to be an agreement between the two within the error limits of small sampling.
Tài liệu tham khảo
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