Hydrodynamic ablation of protoplanetary discs via supernovae

@article{Close2017HydrodynamicAO,
  title={Hydrodynamic ablation of protoplanetary discs via supernovae},
  author={J. L. Close and J. Pittard},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2017},
  volume={469},
  pages={1117-1130}
}
We present three-dimensional simulations of a protoplanetary disc subject to the effect of a nearby (0.3 pc distant) supernova (SN), using a time-dependent flow from a one-dimensional numerical model of the supernova remnant (SNR), in addition to constant peak ram pressure simulations. Simulations are performed for a variety of disc masses and inclination angles. We find disc mass-loss rates that are typically 10−7–10−6 M yr−1 (but they peak near 10−5 M yr−1 during the ‘instantaneous’ stripping… Expand
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