Abundances of the Elements in Sharp‐lined Early‐Type Stars fromIUEHigh‐Dispersion Spectrograms. II. The Nitrogen Deficiency in Mercury‐Manganese Stars-Reference-Cited by-同舟云学术

Abundances of the Elements in Sharp‐lined Early‐Type Stars fromIUEHigh‐Dispersion Spectrograms. II. The Nitrogen Deficiency in Mercury‐Manganese Stars

Published:1999-10-20 Issue:2 Volume:524 Page:974-982
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Roby Scott W.,Leckrone David S.,Adelman Saul J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/524/i=2/a=974/pdf

Reference37 articles.

1. Elemental abundance analyses with coadded Dominion Astrophysical Observatory spectrograms – II. The mercury–manganese stars 53 Tauri, Mu Leporis and Kappa Cancri

2. Elemental abundance analyses with coadded Dominion Astrophysical Observatory spectrograms - III. The superficially normal standard stars Theta Leonis, Tau Herculis and Omicron Pegasi

3. Elemental abundance analyses with coadded DAO spectrograms – IV. Revision of previous analyses

4. Elemental abundance analyses with coadded DAO spectrograms - VI. The mercury-manganese stars Nu Cancri, Iota Coronae Borealis and HR 8349

5. Elemental abundance analyses with DAO spectrograms - VII. The late normal B stars Pi Ceti, 134 Tauri, 21 Aquilae, and Nu Capricorni and the use of Reticon spectra

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