Results 161 to 170 of about 399,848 (263)
SPH Simulations of Protoplanetary Perturbers in Gas Disks [PDF]
Sarah Maddison, Pierre Barge
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Light Echoes of Protoplanetary Disks
Light echoes offer a means of studying protoplanetary disks, including their geometry and composition, even when they are not spatially resolved. We present a test of this approach applied specifically to optically thick, geometrically flared disks ...
Austin J. King, Benjamin C. Bromley
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PHOTOPHORESIS IN A DILUTE, OPTICALLY THICK MEDIUM AND DUST MOTION IN PROTOPLANETARY DISKS [PDF]
Colin P. McNally, Alexander Hubbard
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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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Fossilized condensation lines in the Solar System protoplanetary disk
Alessandro Morbidelli
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On the ionisation fraction in protoplanetary disks III. The effect of X-ray flares on gas-phase chemistry [PDF]
M. Ilgner, Richard P. Nelson
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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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EFFECTS OF RADIONUCLIDES ON THE IONIZATION STATE OF PROTOPLANETARY DISKS AND DENSE CLOUD CORES [PDF]
Toyoharu Umebayashi, Takenori Nakano
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The background temperature of the protoplanetary disk within the first four million years of the Solar System. [PDF]
Schrader DL +3 more
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