146 citations · 371 across the 11 of their papers we have counts for
11 papers
Elemental and Isotopic Yields from T Coronae Borealis: Predictions and Uncertainties
Emma Wallace, Christian Iliadis, Sumner Starrfield
T Coronae Borealis (T CrB) is a symbiotic recurrent nova system expected to undergo its next outburst within the next two years. Recent hydrodynamic simulations have predicted the…
Low-metallicity nova explosions: a site for weak rp-process nucleosynthesis
Athanasios Psaltis, Jordi José, Richard Longland +1
Classical novae are common cataclysmic events involving a binary system of a white dwarf and a main sequence or red giant companion star. In metal-poor environments, these explosio…
Deciphering Spin-Parity Assignments of Nuclear Levels
Christian Iliadis
Spin-parity assignments of nuclear levels are critical for understanding nuclear structure and reactions. However, inconsistent notation conventions and ambiguous reporting in rese…
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…
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…
Sensitivity to Thermonuclear Reaction Rates in Modeling the Abundance Anomalies of NGC 2419
John Dermigny, Christian Iliadis
Abundance anomalies in globular clusters provide strong evidence for multiple stellar populations within each cluster. These populations are usually interpreted as distinct generat…