90 citations · 888 across the 43 of their papers we have counts for
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Gravitoviscous Protoplanetary Discs with a Dust Component. IV. Disc Outer Edges, Spectral Indices, and Opacity Gaps
Vitaly Akimkin, Eduard Vorobyov, Yaroslav Pavlyuchenkov +1
The crucial initial step in planet formation is the agglomeration of micron-sized dust into macroscopic aggregates. This phase is likely to happen very early during the protostella…
ALMA and VLA Observations of EX Lupi in its Quiescent State
Jacob Aaron White, Á. Kóspál, A. G. Hughes +15
Extreme outbursts in young stars may be a common stage of pre-main-sequence stellar evolution. These outbursts, caused by enhanced accretion and accompanied by increased luminosity…
Using HCO isotopologues as tracers of gas depletion in protoplanetary disk gaps
Grigorii V. Smirnov-Pinchukov, Dmitry A. Semenov, Vitaly V. Akimkin +1
The widespread rings and gaps seen in the dust continuum in protoplanetary disks are sometimes accompanied by similar substructures seen in molecular line emission. One example is…
Gravitoviscous protoplanetary disks with a dust component. III. Evolution of gas, dust, and pebbles
Vardan G. Elbakyan, Anders Johansen, Michiel Lambrechts +2
We study the dynamics and growth of dust particles in circumstellar disks of different masses that are prone to gravitational instability during the critical first Myr of their evo…
Chemical modelling of FU Ori protoplanetary disks
Tamara Molyarova, Vitaly Akimkin, Dmitry Semenov +5
Luminosity outbursts of the FUOri type stars, which have a magnitude of and last for decades, may affect chemical composition of the surrounding protoplanetary…
Inhibited Coagulation of Micron-size Dust Due to the Electrostatic Barrier
V. V. Akimkin, A. V. Ivlev, P. Caselli
The collisional evolution of solid material in protoplanetary disks is a crucial step in the formation of planetesimals, comets, and planets. Although dense protoplanetary environm…