Secular brightness variation of the dwarf nova Z Cha during quiescence ⋆
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/242/4/522/18194770/mnras242-0522.pdf
Cited by 20 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. Evolutionary Period Changes for 52 Cataclysmic Variables, and the Failure for the Most-fundamental Prediction of the Magnetic Braking Model;The Astrophysical Journal;2024-05-01
2. The eclipsing accreting white dwarf Z chameleontis as seen with TESS;Monthly Notices of the Royal Astronomical Society;2019-07-31
3. Period changes of cataclysmic variables below the period gap: V2051 Oph, OY Car and Z Cha;New Astronomy;2018-04
4. Survey of period variations of superhumps in SU UMa-type dwarf novae. VII. The seventh year (2014–2015);Publications of the Astronomical Society of Japan;2015-10-14
5. Secular changes in the quiescence of WZ Sagittae: the development of a cavity in the inner disk;Astronomy & Astrophysics;2011-03-18
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