Optical region elemental abundance analyses of B and A stars - I. PI Ceti, 134 Tauri, HR 2154, HR 5780, 21 Aquilae and NU Capricorni-Reference-Cited by-同舟云学术

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Optical region elemental abundance analyses of B and A stars - I. PI Ceti, 134 Tauri, HR 2154, HR 5780, 21 Aquilae and NU Capricorni

Published:1984-02-01 Issue:3 Volume:206 Page:637-648
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Adelman S. J.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/206/3/637/2831798/mnras206-0637.pdf

Cited by 27 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Photospheric aluminium abundances of A-type main-sequence stars;Contributions of the Astronomical Observatory Skalnaté Pleso;2023-11-01

2. Elemental abundance analyses with DAO spectrograms: XXX. The middle B through early A starsξ2Ceti (B9 III), 21 Aquilae (B8 II-III),ιAquilae (B5 III), andιDelphini (A2V);Astronomische Nachrichten;2010-04

3. The magnetic Bp star 36 Lyncis;Astronomy & Astrophysics;2006-09-12

4. Non‐LTE Equivalent Widths for Neiwith Error Estimates;The Astrophysical Journal;1999-07

5. Elemental abundances of the B and A stars — III. Gamma Geninorum, HR 1397, HR 2154, HD 60825 and 7 Sextantis;Monthly Notices of the Royal Astronomical Society;1996-10

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