Planet-induced gas and dust substructure feedbacks on disc thermal structure
Published in MNRAS, 2025
A new paper following up our previous paper Chen et.al 2024. In this paper, we implement multiple dust species into the iterative method. We find the midplane iceline locations are not siginificantly change from our previous gas-only models. We also explore the affects of different turbulent viscosities on the disk thermal structure.
Recommended citation: Chen K., et al., 2025, MNRAS, 541, 2830
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