43 citations · 156 across the 11 of their papers we have counts for
11 papers
Hydrodynamics modeling of the water snow line in young protoplanetary disks with dust-size-dependent opacities
Eduard I. Vorobyov, Anastasiia Topchieva, Aleksandr Skliarevskii +2
Aims. We investigated the properties of the water snow line during the early stages of disk evolution, paying particular attention to the effects of gravitational instability and d…
On the accuracy of mass and size measurements of young protoplanetary disks
Eduard I. Vorobyov, Aleksandr Skliarevskii, Vardan Elbakyan +2
Knowing the masses and sizes of protoplanetary disks is of fundamental importance for the contemporary theories of planet formation. However, their measurements are associated with…
Dust enrichment and growth in the earliest stages of protoplanetary disk formation
E. I. Vorobyov, V. G. Elbakyan, A. Skliarevskii +2
Aims. We numerically investigated dust enrichment and growth during the initial stages of protoplanetary disk formation. A particular objective was to determine the effects of vari…
Primordial dust rings, hidden dust mass, and the first generation of planetesimals in gravitationally unstable protoplanetary disks
Eduard I. Vorobyov, Aleksandr M. Skliarevskii, Manuel Guedel +1
Aims. A new mechanism of dust accumulation and planetesimal formation in a gravitationally unstable disk with suppressed magnetorotational instability is studied and compared with…
Luminosity Outbursts in Interacting Protoplanetary Systems
Aleksandr M. Skliarevskii, Eduard I. Vorobyov
FU Orionis type objects (fuors) are characterized by rapid (tens to hundreds years) episodic outbursts, during which the luminosity increases by orders of magnitude. One of the pos…
Formation of pebbles in (gravito-)viscous protoplanetary disks with various turbulent strengths
Eduard I. Vorobyov, Vardan G. Elbakyan, Anders Johansen +3
Aims. Dust plays a crucial role in the evolution of protoplanetary disks. We study the dynamics and growth of initially sub- dust particles in self-gravitating young protoplane…
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. 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…
The origin of tail-like structures around protoplanetary disks
E. I. Vorobyov, A. M. Skliarevskii, V. G. Elbakyan +4
We study the origin of tail-like structures recently detected around the disk of SU Aurigae and several FU~Orionis-type stars. Dynamic protostellar disks featuring ejections of gas…
Gravitoviscous protoplanetary disks with a dust component. II. Spatial distribution and growth of dust in a clumpy disk
Eduard I. Vorobyov, Vardan G. Elbakyan
Spatial distribution and growth of dust in a clumpy protoplanetary disk subject to vigorous gravitational instability and fragmentation is studied numerically with sub-au resolutio…
Gravitoviscous protoplanetary disks with a dust component. I. The importance of the inner sub-au region
Eduard I. Vorobyov, Aleksandr M. Skliarevskii, Vardan G. Elbakyan +3
The central region of a circumstellar disk is difficult to resolve in global numerical simulations of collapsing cloud cores, but its effect on the evolution of the entire disk can…