Application of the Wesselink method to a non-radially oscillating star-Reference-Cited by-同舟云学术

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Application of the Wesselink method to a non-radially oscillating star

Published:1979-06-01 Issue:2 Volume:187 Page:217-222
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:

Balona L. A.,Stobie R. S.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/187/2/217/3952446/mnras187-0217.pdf

Cited by 28 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. The Telltale Heartbeat: Detection and Characterization of Eccentric Orbiting Planets via Tides on Their Host Star;The Astronomical Journal;2019-01-21

2. Understanding the dynamical structure of pulsating stars: The center-of-mass velocity and the Baade-Wesselink projection factor of theβCephei starαLupi;Astronomy & Astrophysics;2013-05

3. HAS A STAR ENOUGH ENERGY TO EXCITE THE THOUSAND OF MODES OBSERVED WITH CoRoT?;The Astrophysical Journal;2010-01-19

4. The Potential of Multicolor Photometry for Pulsating Subdwarf B Stars;The Astrophysical Journal Supplement Series;2005-12

5. Synthetic photometry for non-radial pulsations in subdwarf B stars;Astronomy & Astrophysics;2004-11-23

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