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Cited article:

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V445 Puppis: Dustier than a Thousand Novae

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The Astrophysical Journal Letters 952 (2) L26 (2023)
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Radio light curves and imaging of the helium nova V445 Puppis reveal seven years of synchrotron emission

M M Nyamai, L Chomiuk, V A R M Ribeiro, et al.
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MCDHF and RCI calculations of energy levels, lifetimes, and transition rates in Si III and Si IV

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Astronomy & Astrophysics 631 A29 (2019)
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Production of Silicon on Mass-increasing White Dwarfs: Possible Origin of High-velocity Features in Type Ia Supernovae

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A new catalogue of Galactic novae: investigation of the MMRD relation and spatial distribution

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OISTER OPTICAL AND NEAR-INFRARED OBSERVATIONS OF TYPE Iax SUPERNOVA 2012Z

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He-accreting white dwarfs: accretion regimes and final outcomes

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Life after eruption – III. Orbital periods of the old novae V365 Car, AR Cir, V972 Oph, HS Pup, V909 Sgr, V373 Sct and CN Vel

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PHASE-RESOLVED INFRARED SPECTROSCOPY AND PHOTOMETRY OF V1500 CYGNI, AND A SEARCH FOR SIMILAR OLD CLASSICAL NOVAE

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ELECTRON-IMPACT EXCITATION OF Cr II: A THEORETICAL CALCULATION OF EFFECTIVE COLLISION STRENGTHS FOR OPTICALLY ALLOWED TRANSITIONS

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On the line intensity ratios of prominent Si II, Si III, and Si IV multiplets

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Line broadening in the Si I, Si II, Si III, and Si IV spectra in the helium plasma

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Helium Nova on a Very Massive White Dwarf: A Revised Light‐Curve Model of V445 Puppis (2000)

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The Astrophysical Journal 684 (2) 1366 (2008)
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