activity
19942005
most citedComplex rotation with internal dissipation. Applications to cosmic-dust alignment and to wobbling comets and asteroids

5 citations · 8 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph2005

Turbulence Statistics from Spectral Line Observations

A. Lazarian

Turbulence is a crucial component of dynamics of astrophysical fluids dynamics, including those of ISM, clusters of galaxies and circumstellar regions. Doppler shifted spectral lin…

astro-ph2005

Cosmic ray transport in MHD turbulence

Huirong Yan, A. Lazarian

Recent advances in understanding of magnetohydrodynamic (MHD) turbulence call for revisions in the picture of cosmic ray transport. In this paper we use recently obtained scaling l…

astro-ph20032 cited

Cosmic Ray Scattering by Compressible Magnetohydrodynamic Turbulence

Huirong Yan, A. Lazarian

Recent advances in understanding of magnetohydrodynamic (MHD) turbulence call for substantial revisions in the picture of cosmic ray transport. In this paper we use recently obtain…

astro-ph20021 cited

The Properties of Compressible MHD and Cosmic Ray Transport

A. Lazarian, Jungyeon Cho, Huirong Yan

Turbulence is the most common state of astrophysical flows. In typical astrophysical fluids, turbulence is accompanied by strong magnetic fields, which has a large impact on the dy…

astro-ph20025 cited

Complex rotation with internal dissipation. Applications to cosmic-dust alignment and to wobbling comets and asteroids

Michael Efroimsky, A. Lazarian, Vladislav Sidorenko

Neutron stars, asteroids, comets, cosmic-dust granules, spacecraft, as well as whatever other freely spinning body dissipate energy when they rotate about any axis different from p…

astro-ph2002

Dust Motions Driven by MHD Turbulence

A. Lazarian, Huirong Yan

We discuss the relative grain motions due to MHD turbulence in interstellar medium. It has been known for decades that turbulent drag is an efficient way to induce grain relative m…