Deriving precise parameters for cool solar-type stars: Optimizing the iron line list

Astronomy and Astrophysics

Volumn 555, Issue , 2013, Pages

  Tsantaki, M ^a,b   Sousa, S G ^a,c   Adibekyan, V Zh ^a   Santos, N C ^a,b   Mortier, A ^a,b   Israelian, G ^c  

^a CENTRO DE ASTROFÍSICA   (Portugal)

^b UNIVERSITY OF PORTO   (Portugal)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

Author keywords

Stars: fundamental parameters; Techniques: spectroscopic

Indexed keywords

ABUNDANCE ANALYSIS; ATMOSPHERIC PARAMETERS; IONIZATION BALANCE; SOLAR TYPE STARS; SPECTROSCOPIC TECHNIQUE; STARS:FUNDAMENTAL PARAMETERS; STELLAR PARAMETERS; TECHNIQUES: SPECTROSCOPIC;

COOLING SYSTEMS; IRON; OPTIMIZATION; SIGNAL TO NOISE RATIO; SPECTROSCOPIC ANALYSIS;

STARS;

EID: 84878462426     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201321103     Document Type: Article

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