Good abundances from bad spectra - I. Techniques

Monthly Notices of the Royal Astronomical Society

Volumn 278, Issue 1, 1996, Pages 146-182

  Bryn Jones, J ^a,b   Gilmore, Gerard ^b   Wyse, Rosemary F G ^b,c,d  

^a CARDIFF UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Methods: data analysis; Stars: abundances; Stars: atmospheres

Indexed keywords

CALIBRATION; SIGNAL TO NOISE RATIO; STARS; SURVEYS; TEMPERATURE;

EFFECTIVE TEMPERATURE; LOW SIGNAL-TO-NOISE RATIO; METHODS. DATA ANALYSIS; SPECTRA'S; STARS ABUNDANCES; STARS: ATMOSPHERE; STELLAR SPECTRA; STELLARS; SURFACE GRAVITY; SYNTHETIC SPECTRA;

IRON;

EID: 1542637389     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/278.1.146     Document Type: Article

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