Elemental abundance analyses with DAO spectrograms. XXVII. The superficially normal stars θ and (A2 IV), ε Del (B6 III), ε Aqr (A1.5 V), and ι and (B9 V)

Astronomy and Astrophysics

Volumn 406, Issue 3, 2003, Pages 975-980

  Kocer, D ^a   Adelman, S J ^b,c   Caliskan, H ^d   Gulliver, A F ^c,e   Tektunali, H Gokmen ^d  

^a ISTANBUL KULTUR UNIVERSITY   (Turkey)

^b THE CITADEL   (United States)

^c NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^d ISTANBUL UNIVERSITY   (Turkey)

^e BRANDON UNIVERSITY   (Canada)

Author keywords

Stars: abundances; Stars: individual: Aqr; Stars: individual: Del; Stars: individual: And; Stars: individual: And

Indexed keywords

ASTRONOMY; ATMOSPHERIC SPECTRA; CHARGE COUPLED DEVICES; OPTICAL SENSORS; SPECTROPHOTOMETERS; VELOCITY;

ELEMENTAL ABUNDANCE; INDIVIDUAL; SPECTROGRAMS; STARS;

GALAXIES;

EID: 0042698662     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030620     Document Type: Article

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