activity
20042026
most citedGlobal magnetohydrodynamical models of turbulence in protoplanetary disks I. A cylindrical potential on a Cartesian grid and transport of solids

83 citations · 226 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2026

Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets

Bhupendra Mishra, Wladimir Lyra, Barry McKernan +3

The outer regions of AGN disks have temperatures similar to those of circumstellar disks, permitting dust condensation. Therefore, planet formation and growth could be active in th…

astro-ph.HE2026

AGN Disks as Supernova Mufflers I: 3D Local Hydrodynamic Models

Harrison E. Cook, Wladimir Lyra, Mordecai-Mark Mac Low +2

Supernova (SN) shocks that originate from stars on orbits embedded in dense active galactic nuclei (AGN) accretion disks evolve differently from those that occur in the interstella…

astro-ph.EP2025

Where are the missing Kuiper Belt binaries?

Wladimir Lyra

In this letter, we call attention to a gap in binaries in the Kuiper belt in the mass range between 10-10 kg, with a corresponding dearth in binaries between…

astro-ph.EP2024★ 11 cited

Planetesimal and planet formation in transient dust traps

Zs. Sándor, O. M. Guilera, Zs. Regály +1

The ring-like structures in protoplanetary discs that are observed in the cold dust emission by ALMA, might be explained by dust aggregates trapped aerodynamically in pressure maxi…

astro-ph.EP2023★ 2 cited

Streaming Instability and Turbulence: Conditions for Planetesimal Formation

Jeonghoon Lim, Jacob B. Simon, Rixin Li +6

The streaming instability (SI) is a leading candidate for planetesimal formation, which can concentrate solids through two-way aerodynamic interactions with the gas. The resulting…

astro-ph2008★ 13 cited

Turbulent stresses as a function of shear rate in a local disk model

A. J. Liljeström, M. J. Korpi, P. J. Käpylä +2

We present local numerical models of accretion disk turbulence driven by the magnetorotational instability with varying shear rate. The resulting turbulent stresses are compared wi…