The new RS CVn binary V1034 Her revisited and the orbital period — activity relation of short-period RS CVn binaries using photometric distortion amplitude-Reference-Cited by-同舟云学术

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The new RS CVn binary V1034 Her revisited and the orbital period — activity relation of short-period RS CVn binaries using photometric distortion amplitude

Published:2012-03-27 Issue:4 Volume:12 Page:433-442
ISSN:1674-4527
Container-title:Research in Astronomy and Astrophysics
language:
Short-container-title:Res. Astron. Astrophys.

Author:

Zhang Li-Yun

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference66 articles.

1. Long-term luminosity variations and period changes in CG Cygni

2. Two-colour photoelectric photometry of UV piscium and fourier analysis of its out-of-eclipse light variations

3. ROTSE All-Sky Surveys for Variable Stars. I. Test Fields

4. A mechanism for orbital period modulation in close binaries

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1. BVR C I C Observations and Analysis of the UV LEO-type Binary, the Pre-WUMa, V1023 Persei;The Astronomical Journal;2020-09-21

2. Physical Parameters of Northern Eclipsing Binaries in the Catalina Sky Survey;The Astrophysical Journal Supplement Series;2019-05-08

3. Chromospheric activity in several single late-type stars;Research in Astronomy and Astrophysics;2015-01-28

4. Magnetic activity and orbital periods of five low-mass eclipsing binaries;Monthly Notices of the Royal Astronomical Society;2014-06-26

5. PHOTOMETRIC PROPERTIES FOR SELECTED ALGOL-TYPE BINARIES. VII. V404 AND WITH MAGNETIC ACTIVITY;The Astronomical Journal;2014-02-11

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