Metal-rich SX Phe stars in theKeplerfield-Reference-Cited by-同舟云学术

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Metal-rich SX Phe stars in theKeplerfield

Published:2016-11-29 Issue:2 Volume:466 Page:1290-1329
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Nemec James M.,Balona Luis A.,Murphy Simon J.,Kinemuchi Karen,Jeon Young-Beom

Funder

Danish National Research Foundation

NASA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/466/2/1290/10867107/stw3072.pdf

Reference241 articles.

1. Adelman S. Proc. IAU Symp. 224, The A-Star Puzzle. Zverko J. Ziznovsky J. Adelman S. J. Weiss W. W. , editors. Kluwer; Dordrecht; 2004. p. 1.

2. The age and interior rotation of stars from asteroseismology

3. Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars

4. On the use of the Fourier transform to determine the projected rotational velocity of line-profile variable B stars

5. The Chemical Composition of the Sun

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