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2006A&A...458..121S - Astronomy and Astrophysics, volume 458, 121-134 (2006/10-4)
Old open clusters as key tracers of Galactic chemical evolution. I. Fe abundances in NGC 2660, NGC 3960, and Berkeley 32.
SESTITO P., BRAGAGLIA A., RANDICH S., CARRETTA E., PRISINZANO L. and TOSI M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): stars: abundances - stars: evolution - Galaxy: disk - open clusters and associations: individual: NGC 2660 - open clusters and associations: individual: NGC 3960 - open clusters and associations: individual: Berkeley 32
Nomenclature: Table 3, col(1): Cl* NGC 3960 SBR cN (Nos c1 to c9). Table 5, col(1): Cl* Berkeley 32 SBR NNN N=10 among (Nos 17-941).
Simbad objects: 35
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