Enhanced mass transfer events trigger the nova eruptions in T CrB by building 95% of the ignition envelope mass on a 1.29 solar-mass white dwarf via a high-viscosity disk.
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The accretion-driven eruption of the recurrent nova T Corona Borealis
Enhanced mass transfer events trigger the nova eruptions in T CrB by building 95% of the ignition envelope mass on a 1.29 solar-mass white dwarf via a high-viscosity disk.