activity
19972026
most citedThe Burst Mode of Protostellar Accretion

381 citations · 5.4k across the 144 of their papers we have counts for

collaborators

143 papers

astro-ph.EP2026

Secular evolution of viscous and self-gravitating protoplanetary discs with magnetic winds

Evgenii R. Redkin, Eduard I. Vorobyov, Paola Pinilla +2

Traditionally, the disc is believed to evolve under the influence of turbulent viscosity, although the importance of this mechanism has recently been questioned. Alternatively, mag…

astro-ph.EP2026

Infall onto the Protoplanetary Disk during the Gravitational Collapse of a Molecular Cloud

E. R. Redkin, E. I. Vorobyov

The development of models for matter infall from a collapsing molecular cloud is an essential part of numerical studies on the formation and evolution of protoplanetary disks. In t…

astro-ph.EP2026

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…

astro-ph.SR2026

Solar-like oscillations in accreting pre-main sequence stars: Insights and prospects

Johannes Jørgensen, Konstanze Zwintz, Ebraheem Farag +2

We present theoretical predictions for solar-like oscillators in the pre-main sequence phase of stellar evolution. Our pre-main sequence models start from a stellar seed of 0.01 so…

astro-ph.EP2025★ 3 cited

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…

astro-ph.EP2025

The Effect of Luminosity Outbursts on the Abundance of Pebbles and Their Ice Mantles in Protoplanetary Disks

Anastasiia Topchieva, Tamara Molyarova, Eduard Vorobyov

Centimeter-sized dust grains-pebbles-are necessary for planetesimal formation via the streaming instability, they play an important role in forming protoplanetary cores and giant p…