The Nova-like Variable WX Centauri and the V Sagittae Phenomenon
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 27 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. Revised ephemeris and orbital period derivative of the supersoft X-ray source CAL 87 based on 34 yr of observations;Monthly Notices of the Royal Astronomical Society;2023-11-27
2. Long-term photometric behavior and orbital period variations in the supersoft X-ray source V617 Sgr;New Astronomy;2023-10
3. The Evolution of the Supersoft X-Ray Source WX Cen Dominated by Magnetic Wind;The Astrophysical Journal;2023-02-01
4. WX Cen is X‐ray quiet: Does this signify a high‐mass or a low‐mass binary?;Astronomische Nachrichten;2022-11
5. Activity of the post-nova V1363 Cygni on long timescales;Publications of the Astronomical Society of Japan;2022-04-22
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