T CrB's 15-year brightening is best explained by a temporary hundredfold increase in mass transfer onto a high-viscosity disk, with the pre-eruption dip caused by an inner disk edge expanding at 0.02 km/s.
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Modeling the high-brightness state of the recurrent nova T CrB as an enhanced mass-transfer event
T CrB's 15-year brightening is best explained by a temporary hundredfold increase in mass transfer onto a high-viscosity disk, with the pre-eruption dip caused by an inner disk edge expanding at 0.02 km/s.