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Cited article:

A Multiwavelength Light-curve Model of the Classical Nova V339 Del: A Mechanism for the Coexistence of Dust Dip and Supersoft X-Rays

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A phenomenological study of the evolution of shock-induced O i emission lines in the spectrum of nova V2891 Cygni

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https://doi.org/10.1093/mnras/stad1914

The RS Oph Outburst of 2021 Monitored in X-Rays with NICER

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V5856 Sagittarii/2016: Broad Multiepoch Spectral Coverage of a Sustained High-luminosity Nova

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Shocks and dust formation in nova V809 Cep

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Photoionization Modeling of the Dusty Nova V1280 Scorpii

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The Astrophysical Journal 925 (2) 187 (2022)
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The 2016 January eruption of recurrent Nova LMC 1968

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Multiwavelength Modeling of the SED of Nova V339 Del: Stopping the Wind and Long-lasting Super-Eddington Luminosity with Dust Emission

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The Astrophysical Journal 878 (1) 28 (2019)
https://doi.org/10.3847/1538-4357/ab1f07