Open clusters as key tracers of Galactic chemical evolution

Astronomy and Astrophysics

Volumn 488, Issue 3, 2008, Pages 943-958

  Sestito, P ^a   Bragaglia, A ^b   Randich, S ^a   Pallavicini, R ^c   Andrievsky, M ^d,e   Korotin, A ^d,e  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI PALERMO   (Italy)

^d ODESSA NATIONAL UNIVERSITY   (Ukraine)

^e Isaac Newton Institute of Chile   (Ukraine)

Author keywords

Galaxy: disk; Galaxy: open clusters and associations: general; Galaxy: open clusters and associations: individual: Berkeley 20, Berkeley 29, Collinder 261, Melotte 66; Stars: abundances; stars: evolution

Indexed keywords

ASTRONOMY; BARIUM; CALCIUM; CHROMIUM; DISKS (STRUCTURAL COMPONENTS); METALLIZING; NICKEL; NICKEL ALLOYS; SILICON; SODIUM; STARS;

ELEMENTAL RATIOS; EQUIVALENT WIDTH; GALACTIC CENTER; GALACTIC CHEMICAL EVOLUTION; GALACTOCENTRIC DISTANCES; GALAXY: DISK; GALAXY: OPEN CLUSTERS AND ASSOCIATIONS: GENERAL; GALAXY: OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: BERKELEY 20, BERKELEY 29, COLLINDER 261, MELOTTE 66; GIANT STARS; LARGE SAMPLE; METALLICITIES; METALLICITY; NEGATIVE SLOPE; NON-LTE; OPEN CLUSTERS; RADIAL DISTRIBUTIONS; RADIAL GRADIENTS; STARS: ABUNDANCES; STARS: EVOLUTION;

CHLORINE COMPOUNDS;

EID: 51949087878     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809650     Document Type: Article

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