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Non-LTE abundance analysis of A-B stars with low rotational velocities – II. Do A-B stars with normal abundances exist?
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Fundamental parameters of some B-type stars using NOAO Indo-U.S. Library
Elemental Abundance Analyses with DAO Spectrograms. XXXVI. The Hot Metallic Line Stars Theta Leonis and Omicron Pegasi
Saul J. Adelman, Austin F. Gulliver and Robert J. Heaton Publications of the Astronomical Society of the Pacific 127(947) 58 (2015) https://doi.org/10.1086/679636
Elemental Abundance Analyses with DAO Spectrograms XXXVII. The Normal A0 IV Star γ Geminorum
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PRECISE ROTATION RATES FOR FIVE SLOWLY ROTATING A STARS
Elemental abundance analyses with DAO spectrograms: XXX. The middle B through early A stars ξ2 Ceti (B9 III), 21 Aquilae (B8 II‐III), ι Aquilae (B5 III), and ι Delphini (A2V)
Chemical Abundances in the Secondary Star of the Black Hole Binary V4641 Sagittarii (SAX J1819.3−2525)
Kozo Sadakane, Akira Arai, Wako Aoki, Nobuo Arimoto, Masahide Takada-Hidai, Takashi Ohnishi, Akito Tajitsu, Timothy C. Beers, Nobuyuki Iwamoto, Nozomu Tominaga, Hideyuki Umeda, Keiichi Maeda and Ken’ichi Nomoto Publications of the Astronomical Society of Japan 58(3) 595 (2006) https://doi.org/10.1093/pasj/58.3.595
Heavy Element Abundances in Late‐B and Early‐A Stars. I. Co‐AddedIUESpectra of HgMn Stars
S. J. Adelman, C. R. Proffitt, G. M. Wahlgren, D. S. Leckrone and L. Dolk The Astrophysical Journal Supplement Series 155(1) 179 (2004) https://doi.org/10.1086/424802
Elemental abundance analyses with the EBASIM spectrograph of the 2.1-m CASLEO Observatory Telescope