A 1.35-solar-mass white dwarf model reproduces the rapid optical rise and fall of nova V1674 Her and gives a distance of about 8.9 kiloparsecs.
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A comprehensive light curve model of the very fast nova V1674 Herculis
A 1.35-solar-mass white dwarf model reproduces the rapid optical rise and fall of nova V1674 Her and gives a distance of about 8.9 kiloparsecs.