2 papers
astro-ph.SR2025
Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It will be the Brightest Classical or Recurrent Nova Ever Observed in X-rays
S. Starrfield, M. Bose, C. E. Woodward +11
T Coronae Borealis (TCrB) is a recurrent nova (RN) with recorded outbursts in 1866, and 1946 and possible outbursts in 1217 and 1787. It is predicted to explode again in 2025 or 20…
astro-ph.GA2023
A two-component clumpy model for the shell evolution of classical novae: the case of V5668 Sgr
Zulema Abraham, Larissa Takeda, Pedro P. B. Beaklini +4
The shell of the classical nova V5668 Sgr was resolved by ALMA at the frequency of 230 GHz 927 days after eruption, showing that most of the continuum bremsstrahlung emission origi…