Hints for Icy Pebble Migration Feeding an Oxygen-rich Chemistry in the Inner Planet-forming Region of Disks

@article{Banzatti2020HintsFI,
  title={Hints for Icy Pebble Migration Feeding an Oxygen-rich Chemistry in the Inner Planet-forming Region of Disks},
  author={A. Banzatti and I. Pascucci and A. Bosman and P. Pinilla and C. Salyk and G. Herczeg and K. Pontoppidan and I. Vazquez and A. Watkins and S. Krijt and N. Hendler and F. Long},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2020}
}
We present a synergic study of protoplanetary disks to investigate links between inner disk gas molecules and the large-scale migration of solid pebbles. The sample includes 63 disks where two types of measurements are available: i) spatially-resolved disk images revealing the radial distribution of disk pebbles (mm-cm dust grains), from millimeter observations with ALMA or the SMA, and ii) infrared molecular emission spectra as observed with Spitzer. The line flux ratios of H2O with HCN, C2H2… Expand
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