New binary parameters for the symbiotic recurrent nova T Coronae Borealis
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/296/1/77/
Cited by 51 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. Accretion in the recurrent nova T CrB: Linking the superactive state to the predicted outburst;Astronomy & Astrophysics;2023-12
2. Symbiotic Star T CrB as an Extreme SU UMa–type Dwarf Nova;The Astrophysical Journal Letters;2023-08-01
3. Chemical abundance analysis of symbiotic giants. Metallicity and CNO abundance patterns in 14 northern S-type systems;Monthly Notices of the Royal Astronomical Society;2023-07-31
4. The B & V light curves for recurrent nova T CrB from 1842–2022, the unique pre- and post-eruption high-states, the complex period changes, and the upcoming eruption in 2025.5 ± 1.3;Monthly Notices of the Royal Astronomical Society;2023-03-14
5. White Dwarf—Red Giant Star Binaries as Type Ia Supernova Progenitors: With and without Magnetic Confinement;The Astrophysical Journal Letters;2022-12-01
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