2 citations · 2 across the 3 of their papers we have counts for
3 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.SR2024
Hydrodynamic Simulations of Oxygen-Neon Classical Novae as Galactic Li Producers and Potential Accretion Induced Collapse Progenitors
Sumner Starrfield, Maitrayee Bose, Christian Iliadis +3
We report on studies of Classical Nova (CN) explosions where we follow the evolution of thermonuclear runaways (TNRs) on oxygen-neon (ONe) white dwarfs (WDs). Using NOVA, a one-dim…
astro-ph.SR2020★ 2 cited
Hydrodynamic Simulations of Classical Novae; CO and ONe White Dwarfs are Supernova Ia Progenitors
S. Starrfield, M. Bose, C. Iliadis +3
Cataclysmic Variables (CVs) and Symbiotic Binaries are close (or not so close) binary star systems which contain both a white dwarf (WD) primary and a larger cooler secondary star…