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Millimeter-sized Dust Grains Appear Surviving the Water-sublimating Temperature in the Inner 10 au of the FU Ori Disk
Hauyu Baobab Liu, An-Li Tsai, Wen Ping Chen +10
Previous observations have shown that the 10 au, 400 K hot inner disk of the archetypal accretion outburst young stellar object, FU Ori, is dominated by viscous…
Restoration of the Parameters of a Gas-Dust Disk Based on Its Synthetic Images
A. M. Skliarevskii, Ya. N. Pavlyuchenkov, E. I. Vorobyov
The topic of the present study is combining a dynamic model of a protoplanetary disk with the computations of radiation transfer for obtaining synthetic spectra and disk images sui…
Gravitoviscous protoplanetary disks with a dust component. V. The dynamic model for freeze-out and sublimation of volatiles
Tamara Molyarova, Eduard I. Vorobyov, Vitaly Akimkin +3
The snowlines of various volatile species in protoplanetary disks are associated with abrupt changes in gas composition and dust physical properties. Volatiles may affect dust grow…
Simulations of Dynamical Gas-Dust Circumstellar Disks: Going Beyond the Epstein Regime
Olga P. Stoyanovskaya, Fedor A. Okladnikov, Eduard I. Vorobyov +2
In circumstellar disks, the size of dust particles varies from submicron to several centimeters, while planetesimals have sizes of hundreds of kilometers. Therefore, various regime…