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- W1526106927 abstract "Protoplanetary disks heated by radiation from the central star are found to be unstable. We calculate the quasi‐static thermal evolution of irradiated disks by directly integrating the optical depths to determine the optical surface and the total emitting area‐filling factor of surface dust. We show that, in disks with modest mass accretion rates, thermal waves are spontaneously and continually excited in the outer disk, and propagate inward through the planet‐forming domains. The viscous heating due to higher mass accretion stabilizes the instability. In passive protostellar disks, these waves induce a significant change in spectral energy distributions (SEDs). The transitory peaks and troughs in the potential vorticity distribution may also excite vortices in the planet‐forming regions." @default.
- W1526106927 created "2016-06-24" @default.
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- W1526106927 date "2009-01-01" @default.
- W1526106927 modified "2023-10-18" @default.
- W1526106927 title "Thermally Induced Waves in Protoplanetary Disks and Their Implication for Planetary Formation" @default.
- W1526106927 doi "https://doi.org/10.1063/1.3215870" @default.
- W1526106927 hasPublicationYear "2009" @default.
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