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Unevolved Li-rich stars at low metallicity: A possible formation pathway through novae
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DW Cnc: a micronova with a negative superhump and a flickering spin
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Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It Will Be the Brightest Classical or Recurrent Nova Ever Observed in X-Rays*
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A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii
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Mariko Kato, Hideyuki Saio and Izumi Hachisu Publications of the Astronomical Society of Japan 76(4) 666 (2024) https://doi.org/10.1093/pasj/psae038
Thermonuclear 28P(p, γ)29S reaction rate and astrophysical implication in ONe nova explosion
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Expected evolution of the binary system PTF J2238+743015.1
Nucleosynthesis in Type Ia Supernovae, Classical Novae, and Type I X-Ray Bursts. A Primer on Stellar Explosions
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Novae: An Important Source of Lithium in the Galaxy
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Progress on nuclear reaction rates affecting the stellar production of 26Al
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Hydrogen Burning of 29Si and Its Impact on Presolar Stardust Grains from Classical Novae
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Localized thermonuclear bursts from accreting magnetic white dwarfs
Study of 2021 outburst of the recurrent nova RS Ophiuchi: Photoionization and morphokinematic modelling
Ruchi Pandey, Gesesew R Habtie, Rahul Bandyopadhyay, et al. Monthly Notices of the Royal Astronomical Society 515(3) 4655 (2022) https://doi.org/10.1093/mnras/stac2079
Triggering micronovae through magnetically confined accretion flows in accreting white dwarfs
S Scaringi, P J Groot, C Knigge, J-P Lasota, D de Martino, Y Cavecchi, D A H Buckley and M E Camisassa Monthly Notices of the Royal Astronomical Society: Letters 514(1) L11 (2022) https://doi.org/10.1093/mnrasl/slac042
Detection of 7Be ii in the Classical Nova V5669 Sgr (Nova Sagittarii 2015 No.3)
Carbon–Oxygen Classical Novae Are Galactic 7Li Producers as well as Potential Supernova Ia Progenitors
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A unified theory of cataclysmic variable evolution from feedback-dominated numerical simulations