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Cited article:

THE CHEMICAL COMPOSITION OFρPUPPIS AND THE SIGNS OF ACCRETION IN THE ATMOSPHERES OF B–F-TYPE STARS

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The Astronomical Journal 149 (2) 59 (2015)
https://doi.org/10.1088/0004-6256/149/2/59

Fundamental parameters of eight Am stars: comparing observations with theory★

G. Catanzaro and V. Ripepi
Monthly Notices of the Royal Astronomical Society 441 (2) 1669 (2014)
https://doi.org/10.1093/mnras/stu674

Lithium, Sodium, and Potassium Abundances in Sharp-Lined A-Type Stars

Yoichi Takeda, Dong-Il Kang, Inwoo Han, Byeong-Cheol Lee, Kang-Min Kim, Satoshi Kawanomoto and Naoko Ohishi
Publications of the Astronomical Society of Japan 64 (2) (2012)
https://doi.org/10.1093/pasj/64.2.38

LOOKING FOR A CONNECTION BETWEEN THE Am PHENOMENON AND HYBRID δ Sct -γ Dor PULSATION: DETERMINATION OF THE FUNDAMENTAL PARAMETERS AND ABUNDANCES OF HD 114839 AND BD +18 4914

M. Hareter, L. Fossati, W. Weiss, et al.
The Astrophysical Journal 743 (2) 153 (2011)
https://doi.org/10.1088/0004-637X/743/2/153

THE ATMOSPHERE PARAMETERS AND THE LINE PROFILE VARIATIONS OF ρ PUPPIS

A.V. Yushchenko, T.N. Dorokhova, V.F. Gopka, et al.
Journal of The Korean Astronomical Society 43 (3) 65 (2010)
https://doi.org/10.5303/JKAS.2010.43.3.065

Late stages of the evolution of A-type stars on the main sequence: comparison between observed chemical abundances and diffusion models for 8 Am stars of the Praesepe cluster

L. Fossati, S. Bagnulo, R. Monier, et al.
Astronomy & Astrophysics 476 (2) 911 (2007)
https://doi.org/10.1051/0004-6361:20078320