Gravitoviscous Protoplanetary Disks with a Dust Component. V. The Dynamic Model for Freeze-out and Sublimation of Volatiles

نویسندگان

چکیده

Abstract The snowlines of various volatile species in protoplanetary disks are associated with abrupt changes gas composition and dust physical properties. Volatiles may affect growth, as they cover grains icy mantles that can change the fragmentation velocity grains. In turn, coagulation, fragmentation, drift through disk contribute to redistribution volatiles between ice phases. Here we present hydrodynamic model FEOSAD for two populations dynamics. We compute spatial distributions major molecules (H 2 O, CO , CH 4 CO) gas, on small grown dust, analyze over initial 0.5 Myr evolution. show most arrives surface coagulation Spiral structures rings forming disk, well photodissociation outer regions, lead formation complex snowline shapes multiple each species. During considered evolution, shift closer star, their final position being a factor 4–5 smaller than at epoch. demonstrate tend collect vicinity snowlines, both phases, leading thick potentially important size is affected by lower bare higher turbulent viscosity.

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2021

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/abe2b0