Long-term luminosity variations and period changes in CG Cygni-Reference-Cited by-同舟云学术

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Long-term luminosity variations and period changes in CG Cygni

Published:2004-05-28 Issue:2 Volume:420 Page:595-604
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Afşar M.,Heckert P. A.,İbanoǧlu C.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20040115/pdf

Reference47 articles.

1. Afsar, M., & Ibanoglu, C. 2000, IBVS, 4979

2. A mechanism for orbital period modulation in close binaries

3. Banks, T. S. 1989, Masters Thesis, Victoria Univ., Wellington

4. Beckert, D., Cox, D., Gordon, S., Ledlow, M., & Zeilik, M. 1989, IBVS, 3398

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1. Characteristics of Long-Term Spot Activity on Several Late-Spectral-Type Stars;Astronomy Reports;2023-09

2. PECULIARITIES OF LONG-TERM SPOT ACTIVITY OF SOME LATE SPECTRAL-TYPE STARS;Астрономический журнал;2023-09-01

3. Physical Properties of Three Eclipsing Binaries of V Crt, WY Cnc and CG Cyg with Radio Radiation;Universe;2022-10-24

4. Orbital Period Investigation of the RS CVn-Type Binary CG Cygni;Publications of the Astronomical Society of Japan;2012-12-25

5. Spot activity of the binary CG Cyg: Observations during maximum spottedness;Astronomy Reports;2012-04

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