Self-consistent simulations show that planet-carved gaps heat the disk midplane by tens of Kelvin, while dust rings cool it, shifting and multiplying the icelines of water, CO2, and CO compared to smooth-disk models.
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Planet-induced Gas and Dust Substructure Feedbacks on Disk Thermal Structure
Self-consistent simulations show that planet-carved gaps heat the disk midplane by tens of Kelvin, while dust rings cool it, shifting and multiplying the icelines of water, CO2, and CO compared to smooth-disk models.