Dust-gas chemistry in AGB outflows: Chemical modelling of dust-gas chemistry within AGB outflows I. Effect on the gas-phase

@article{Sande2019DustgasCI,
  title={Dust-gas chemistry in AGB outflows: Chemical modelling of dust-gas chemistry within AGB outflows I. Effect on the gas-phase},
  author={M. V. D. Sande and C. Walsh and T. P. Mangan and L. Decin},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2019}
}
  • M. V. D. Sande, C. Walsh, +1 author L. Decin
  • Published 2019
  • Physics
  • arXiv: Solar and Stellar Astrophysics
  • Chemical modelling of AGB outflows is typically focused on either non-thermodynamic equilibrium chemistry in the inner region or photon-driven chemistry in the outer region. We include, for the first time, a comprehensive dust-gas chemistry in our AGB outflow chemical kinetics model, including both dust-gas interactions and grain-surface chemistry. The dust is assumed to have formed in the inner region, and follows an interstellar-like dust-size distribution. Using radiative transfer modelling… CONTINUE READING
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