Open AccessFractional yields inferred from halo and thick disk stars (Serb. Astron. J. - 187 (2013), 19)
Author(s) -
R. Caimmi
Publication year - 2014
Publication title -
serbian astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.196
H-Index - 16
eISSN - 1820-9289
pISSN - 1450-698X
DOI - 10.2298/saj1488099e
Subject(s) - astron , physics , astrophysics , halo , sign (mathematics) , stars , yield (engineering) , astronomy , galaxy , mathematical analysis , mathematics , thermodynamics
Due to a wrong sign in a computer code, theoretical yield ratios have been recalculated. Related changes affect only Figs. 12-13, where theoretical yield ratios are represented as vertical bands. The correct figures are provided and differences with respect to the earlier version are mentioned. Minor corrections are also shown
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