Analysis of medium resolution spectra by automated methods -Application to M 55 and ω Centauri

Astronomy and Astrophysics

Volumn 436, Issue 1, 2005, Pages 379-390

  Willemsen, P G ^a   Hilker, M ^a   Kayser, A ^a,b   Bailer Jones, C A L ^c  

^a UNIVERSITY OF BONN   (Germany)

^b UNIVERSITY OF BASEL   (Switzerland)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Globular clusters: individual: Centauri; Globular clusters: individual: M 55; Methods: data analysis; Stars: abundances; Stars: fundamental parameters; Techniques: spectroscopic

Indexed keywords

DATA REDUCTION; OPTICAL RESOLVING POWER; PARAMETER ESTIMATION; PHOTOMETRY; PROBLEM SOLVING;

METHODS: DATA ANALYSIS; STARS: ABUNDANCES; STARS: FUNDAMENTAL PARAMETERS; TECHNIQUES: SPECTROSCOPIC;

SPECTRUM ANALYSIS;

EID: 24644480074     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041974     Document Type: Article

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