Filament Formation due to Diffusive Instabilities in Dusty Protoplanetary Disks
We report the finding of a new, local diffusion instability in a protoplanetary disk which can operate in a dust fluid, subject to mass diffusion, shear viscosity, and dust–gas drag, provided the diffusivity, viscosity, or both, decrease sufficiently ...
Konstantin Gerbig+2 more
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Diversity of planetary systems from evolution of solids in protoplanetary disks [PDF]
K. Kornet+2 more
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Protoplanetary Disks in the Nearest Star-Forming Cloud: Mid-Infrared Imaging and Optical Spectroscopy of MBM 12 Members [PDF]
Ray Jayawardhana+4 more
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We analyze near-infrared integral field spectropolarimetry of the AB Aurigae protoplanetary disk and protoplanet (AB Aur b), obtained with SCExAO/CHARIS in 22 wavelength channels covering the J , H , and K passbands ( λ _0 = 1.1–2.4 μ m) over angular ...
Erica Dykes+23 more
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Two-dimensional distributions and column densities of gaseous molecules in protoplanetary disks [PDF]
Yuri Aikawa, Eric Herbst
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JWST MIRI MRS Images of Disk Winds, Water, and CO in an Edge-on Protoplanetary Disk
We present JWST MIRI MRS observations of the edge-on protoplanetary disk around the young subsolar-mass star Tau 042021, acquired as part of the Cycle 1 GO program “Mapping Inclined Disk Astrochemical Signatures.” These data resolve the mid-IR spatial ...
Nicole Arulanantham+16 more
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Planetary Torques as the Viscosity of Protoplanetary Disks [PDF]
Jeremy Goodman, Roman R. Rafikov
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Halting Planet Migration in the Evacuated Centers of Protoplanetary Disks [PDF]
Marc J. Kuchner, M. Lecar
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Structure and Instabilities of an Irradiated Viscous Protoplanetary Disk [PDF]
Hideko Nomura
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Low-mass Stars: Their Protoplanetary Disk Lifetime Distribution
While most protoplanetary disks lose their gas within less than 10 Myr, individual disk lifetimes vary from 5 Myr. The next challenge is to quantitatively link the diversity of disk lifetimes to the diversity in planets.
Susanne Pfalzner, Furkan Dincer
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