Deriving temperature, mass, and age of evolved stars from high-resolution spectra*: Application to field stars and the open cluster IC 4651

Astronomy and Astrophysics

Volumn 475, Issue 3, 2007, Pages 981-989

  Biazzo, K ^a,b   Pasquini, L ^b   Girardi, L ^c   Frasca, A ^a   Da Silva, L ^d   Setiawan, J ^e   Marilli, E ^a   Hatzes, A P ^f   Catalano, S ^a  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^d OBSERVATÓRIO NACIONAL   (Brazil)

^e MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^f Tauterburg   (Germany)

Author keywords

Galaxy: open cluster and associations: individual: IC 4651; Stars: late type; Techniques: spectroscopic

Indexed keywords

CALIBRATION; CLUSTER ANALYSIS; SPECTROSCOPIC ANALYSIS; SPECTRUM ANALYSIS;

HIGH-RESOLUTION SPECTRA; LINE-DEPTH RATIOS (LDR); OPEN CLUSTER; SPECTRAL SYNTHESIS;

STARS;

EID: 36549033323     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20077374     Document Type: Article

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