A spectroscopic study of the open cluster NGC 6475 (M 7)

Astronomy and Astrophysics

Volumn 504, Issue 3, 2009, Pages 845-852

  Villanova, S ^a   Carraro, G ^b   Saviane, I ^b  

^a UNIVERSITY OF CONCEPCIÓN   (Chile)

^b EUROPEAN SOUTHERN OBSERVATORY   (Chile)

Author keywords

Galaxy: open clusters and associations: individual: NGC 6475; Stars: abundances

Indexed keywords

ATMOSPHERIC PARAMETERS; BALMER LINES; BASIC PARAMETERS; CHEMICAL ABUNDANCE; CHEMICAL COMPOSITIONS; CHEMICAL CONTENT; CHEMICAL EVOLUTION; COOL STARS; EQUIVALENT WIDTH; EVOLUTIONARY PHASE; FUNDAMENTAL PARAMETERS; GALAXY: OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: NGC 6475; HIGH-RESOLUTION SPECTRA; HYPERFINE STRUCTURE; ISOCHRONES; KEY OBJECT; LIGHT ELEMENTS; LUMINOSITY CLASS; METALLICITIES; OPEN CLUSTERS; SPECTRAL LINE; SPECTROSCOPIC STUDIES; STARS: ABUNDANCES; STELLAR EVOLUTIONS; SURFACE CHEMICALS; SYSTEMATIC EFFECTS;

BARIUM; CHEMICAL ELEMENTS; GALAXIES; HELIUM; SODIUM; SPECTROSCOPIC ANALYSIS; SPECTROSCOPY;

STARS;

EID: 70349491264     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811507     Document Type: Article

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