On the Gaiiand GaiiiResonance Lines and the Implication for Chemical Stratification in HgMn Stars-Reference-Cited by-同舟云学术

On the Gaiiand GaiiiResonance Lines and the Implication for Chemical Stratification in HgMn Stars

Published:2005-11 Issue:5 Volume:130 Page:2312-2317
ISSN:0004-6256
Container-title:The Astronomical Journal
language:en
Short-container-title:Astron J

Author:

Nielsen K. E.,Wahlgren G. M.,Proffitt C. R.,Leckrone D. S.,Adelman S. J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference30 articles.

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

2. Heavy Element Abundances in Late‐B and Early‐A Stars. I. Co‐AddedIUESpectra of HgMn Stars

3. Alecian, G. & Artru, M. C. 1988, in IAU Symp. 132, The Impact of Very High S/N Spectroscopy on Stellar Physics, ed. G. Cayrel de Strobel & M. Spite (Dordrecht: Kluwer), 235

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