The pure dipole pulsation mode of the rapidly oscillating Ap star α Cir: determination of the rotation period, and evidence for frequency variability-Reference-Cited by-同舟云学术

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The pure dipole pulsation mode of the rapidly oscillating Ap star α Cir: determination of the rotation period, and evidence for frequency variability

Published:1994-10 Issue:3 Volume:270 Page:674-686
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Kurtz D. W.,Sullivan D. J.,Martinez Peter,Tripe P.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/270/3/674/18199856/mnras270-0674.pdf

Cited by 50 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. A benchmark rapidly oscillating chemically peculiar (roAp) star: α Cir;Astronomy & Astrophysics;2024-08

2. TESS cycle 1 observations of roAp stars with 2-min cadence data;Monthly Notices of the Royal Astronomical Society;2021-05-31

3. New BRITE-Constellation observations of the roAp star α Cir;Astronomy & Astrophysics;2020-10

4. The Large Far Ultraviolet Variations of α Cir A and α Cir B as Recorded by IUE and FUSE;Research Notes of the AAS;2020-09-22

5. SALT HRS Capabilities for Time Resolved Pulsation Analysis: A Test with the roAp Star α Circini*;Publications of the Astronomical Society of the Pacific;2020-09-02

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