Population synthesis of accreting white dwarfs: rates and evolutionary pathways of H and He novae

@inproceedings{Kemp2021PopulationSO,
  title={Population synthesis of accreting white dwarfs: rates and evolutionary pathways of H and He novae},
  author={A. J. Kemp and A. Karakas and A. Casey and R. Izzard and A. Ruiter and P. Agrawal and F. Broekgaarden and Karel D. Temmink},
  year={2021}
}
Novae are some of the most commonly detected optical transients and have the potential to provide valuable information about binary evolution. Binary population synthesis codes have emerged as the most effective tool for modelling populations of binary systems, but such codes have traditionally employed greatly simplified nova physics, precluding detailed study. In this work, we implement a model treating H and He novae as individual events into the binary population synthesis code binary_c… Expand

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