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)

DOI	Resolve DOI: https://doi.org/10.1051/0004-6361:20030620
Author	Search for: Kocer, D.; Search for: Adelman, S. J.¹; Search for: Caliskan, H.; Search for: Gulliver, A. F.¹; Search for: Tektunali, H. Gokmen
Affiliation	National Research Council of Canada. NRC Herzberg Institute of Astrophysics
Format	Text, Article
Subject	stars: abundances; stars: individual: θ And; stars: individual: ϵ Del; stars: individual: ϵ Aqr; stars: individual: ι And
Abstract	The superficially normal stars θ And (A2 V), ϵ Del (B6 III), ϵ Aqr (A1.5 V), and ι And (B9 V), which have rotationally broadened line profiles, are analyzed in a manner consistent with previous studies of this series using 2.4 Å mm-1 spectrograms obtained with CCD detectors and S/N ≥ 200. Their variable radial velocities strongly suggest they are spectroscopic binaries. As no evidence is seen for lines of their companions they are analyzed as single stars. Their derived abundances are generally near solar. But those for θ And suggest that it is possibly a fast rotating Am star.
Publication date	2003-11-17
Publisher	EDP Sciences
In	Astronomy & Astrophysics 406, no. 3 (17 November 2003): 975–980.
Language	English
Peer reviewed	Yes
NPARC number	9724445
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Record identifier	250a346d-0078-43e9-a353-ee8aacfd362d
Record created	2009-07-17
Record modified	2024-04-26