245 citations · 3.9k across the 125 of their papers we have counts for
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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…
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…
Snowflakes in a furnace: formation of CO and dust in a recurrent nova eruption
D. P. K. Banerjee, C. E. Woodward, V. Joshi +7
We report the detection of carbon monoxide (CO) and dust, formed under hostile conditions, in recurrent nova V745 Sco about 8.7 days after its 2014 outburst. The formation of molec…
V445 Puppis -- Dustier than a Thousand Novae
D. P. K. Banerjee, A. Evans, C. E. Woodward +4
V445 Puppis, the only known Galactic helium nova, is a unique test-bed to verify supernova (SN) theories in the single degenerate channel that involve a white dwarf (WD) accreting…
Infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco
A. Evans, D. P. K. Banerjee, C. E. Woodward +5
We present near-infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco, over the period from 5.2 to 45.4 days after outburst. This is the most intensive infrared st…
Infrared spectroscopy of the 2019 eruption of the recurrent nova V3890 Sgr: separation into equatorial and polar winds revealed
A. Evans, T. R. Geballe, C. E. Woodward +4
We present infrared spectroscopy of the 2019 eruption of the recurrent nova V3890 Sgr, obtained over the period 5.1-46.3 days after the eruption. The spectrum of the red giant beca…