An explanation of the long-term behaviour of the pulsation amplitudes of the β Cephei star 16 (EN) Lacertae-Reference-Cited by-同舟云学术

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An explanation of the long-term behaviour of the pulsation amplitudes of the β Cephei star 16 (EN) Lacertae

Published:1996-10 Issue:3 Volume:282 Page:853-862
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Jerzykiewicz M.,Pigulski A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/282/3/853/

Cited by 14 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 2003–2004 multisite photometric campaign for the β Cephei and eclipsing star 16 (EN) Lacertae with an appendix on 2 Andromedae, the variable comparison star;Monthly Notices of the Royal Astronomical Society;2015-09-24

2. Mode Parameters ofδScuti Stars V830 Her and HD 163032 with Four-Year Data from the Taiwan Automated Telescope Network;Publications of the Astronomical Society of the Pacific;2013-01

3. A multisite photometric study of two unusual β Cep stars: the magnetic V2052 Oph and the massive rapid rotator V986 Oph;Monthly Notices of the Royal Astronomical Society;2012-07-16

4. β Cephei stars in the ASAS-3 data;Astronomy & Astrophysics;2007-12-04

5. A new analysis of the radial velocity variations of the eclipsing and spectroscopic binary EN Lacertae;Astronomy & Astrophysics;2001-02

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