Carbon-Oxygen Classical Novae are Galactic $^7$Li Producers as well as Potential Supernova Ia Progenitors

@article{Starrfield2019CarbonOxygenCN,
  title={Carbon-Oxygen Classical Novae are Galactic \$^7\$Li Producers as well as Potential Supernova Ia Progenitors},
  author={S. Starrfield and M. Bose and C. Iliadis and W. Hix and C. Woodward and R. Wagner},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2019}
}
We report on studies of Classical Nova (CN) explosions where we follow the evolution of thermonuclear runaways (TNRs) on Carbon Oxygen (CO) white dwarfs (WDs). We vary both the mass of the WD (from 0.6 M$_\odot$ to 1.35 M$_\odot$) and the composition of the accreted material. Our simulations are guided by the results of multi-dimensional studies of TNRs in WDs that find sufficient mixing with WD core material occurs after the TNR is well underway, reaching levels of enrichment that agree with… Expand
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