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Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs
Triantafyllos Kormpakis, Manuel Linares and Jordi José Monthly Notices of the Royal Astronomical Society 540(3) 2305 (2025) https://doi.org/10.1093/mnras/staf853
Hubble Space Telescope Far-UV Spectroscopy of the Short Orbital Period Recurrent Nova CI Aql: Implications for White Dwarf Mass Evolution
Edward M. Sion, R. E. Wilson, Patrick Godon, Sumner Starrfield, Robert E. Williams and M. J. Darnley The Astrophysical Journal 872(1) 68 (2019) https://doi.org/10.3847/1538-4357/aafb0b
Self-gravitating Semi-transparent Circumstellar Disks: An Analytic Model
Aykut Özdönmez, Tolga Güver, Antonio Cabrera-Lavers and Tansel Ak Monthly Notices of the Royal Astronomical Society 461(2) 1177 (2016) https://doi.org/10.1093/mnras/stw1362
OUTBURST-RELATED PERIOD CHANGES OF RECURRENT NOVA CI AQUILAE
D. I. Sahman, V. S. Dhillon, T. R. Marsh, et al. Monthly Notices of the Royal Astronomical Society 433(2) 1588 (2013) https://doi.org/10.1093/mnras/stt830
Spectroscopic observations of the recurrent nova CI Aquilae during the 2000 outburst
Seiichiro Kiyota, Taichi Kato and Hitoshi Yamaoka Publications of the Astronomical Society of Japan 56(sp1) S193 (2004) https://doi.org/10.1093/pasj/56.sp1.S193
Variable Star Network: World Center for Transient Object Astronomy and Variable Stars
Taichi Kato, Makoto Uemura, Ryoko Ishioka, Daisaku Nogami, Chatief Kunjaya, Hajime Baba and Hitoshi Yamaoka Publications of the Astronomical Society of Japan 56(sp1) S1 (2004) https://doi.org/10.1093/pasj/56.sp1.S1
High-speed photometry of the recurrent nova IM Normae
A New Clue to the Transition Mechanism between Optical High and Low States of the Supersoft X‐Ray Source RX J0513.9−6951, Implied By the Recurrent Nova CI Aquilae 2000 Outburst Model
The Recurrent Nova U Scorpii in the 1999 Outburst: the First Detection of a Significant Orbital-Period Change
Katsura Matsumoto, Taichi Kato and Izumi Hachisu Publications of the Astronomical Society of Japan 55(1) 297 (2003) https://doi.org/10.1093/pasj/55.1.297
A Limit Cycle Model For Long‐Term Optical Variations of V Sagittae: The Second Example of Accretion Wind Evolution