B-type supergiants in the SMC: Chemical compositions and comparison of static and unified models

Astronomy and Astrophysics

Volumn 434, Issue 3, 2005, Pages 1125-1137

  Dufton, P L ^a   Ryans, R S I ^a   Trundle, C ^b   Lennon, D J ^c   Hubeny, I ^d   Lanz, T ^e   Allende Prieto, C ^f  

^a QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^b Insitituto de Astrofísica   (Spain)

^c ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^d UNIVERSITY OF ARIZONA   (United States)

^e Bldg 142   (United States)

^f The University of Texas at Austin   (United States)

Author keywords

Galaxies: Magellanic Clouds; Stars: Abundances; Stars: early type; Stars: supergiants

Indexed keywords

ATMOSPHERIC SPECTRA; ATMOSPHERICS; CLOUDS; COMPOSITION; DATA REDUCTION; ERROR ANALYSIS; GALAXIES; MATHEMATICAL MODELS; PARAMETER ESTIMATION;

ABUNDANCES - STARS; EARLY-TYPE - STARS; MAGELLANIC CLOUDS - STARS; SUPERGIANTS;

ASTRONOMY;

EID: 18444363317     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042530     Document Type: Article

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