THE CHEMICAL COMPOSITION OFρPUPPIS AND THE SIGNS OF ACCRETION IN THE ATMOSPHERES OF B

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

Published:2015-01-19 Issue:2 Volume:149 Page:59
ISSN:1538-3881
Container-title:The Astronomical Journal
language:
Short-container-title:AJ

Author:

Yushchenko Alexander V.,Gopka Vira F.,Kang Young-Woon,Kim Chulhee,Lee Byeong-Cheol,Yushchenko Volodymyr A.,Dorokhova Tatyana N.,Doikov Dmytry N.,Pikhitsa Petro V.,Hong Kyeongsoo,Kim Sungeun,Lee Jae-Woo,Rittipruk Pakakaew

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1538-3881/149/i=2/a=59/pdf

Reference111 articles.

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

2. Radiative accelerations in stars: The effect of Zeeman splitting

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