Old open clusters as key tracers of Galactic chemical evolution I. Fe abundances in NGC 2660, NGC 3960, and Berkeley 32

Astronomy and Astrophysics

Volumn 458, Issue 1, 2006, Pages 121-134

  Sestito, P ^a,b,c   Bragaglia, A ^c   Randich, S ^b   Carretta, E ^c   Prisinzano, L ^a   Tosi, M ^c  

^a INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^c OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

Author keywords

Galaxy: disk; Open clusters and associations: individual: Berkeley 32; Open clusters and associations: individual: NGC 2660; Open clusters and associations: individual: NGC 3960; Stars: abundances; Stars: evolution

Indexed keywords

ASTROPHYSICS; IRON; OPTICAL RESOLVING POWER; PROJECT MANAGEMENT; SOLAR ENERGY; SPECTRUM ANALYSIS;

GALAXY: DISK; OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: BERKELEY 32; OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: NGC 2660; OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: NGC 3960; STARS: ABUNDANCES; STARS: EVOLUTION;

GALAXIES;

EID: 33750260821     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065175     Document Type: Article

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