Supernovae (SNe) explosions are thought to be an important source of dust in galaxies. At
the same time strong shocks from SNe are known as an efficient mechanism of dust …

Context. Dust grain dynamics in molecular clouds is regulated by its interplay with
supersonic turbulent gas motions. The conditions under which interstellar dust grains …

This paper reports the findings from a three-dimensional direct numerical simulation
conducted to investigate the turbulent flame behaviors of premixed high-hydrogen content …

A series of direct numerical simulations (DNSs) of forced compressible isothermal
turbulence in a periodic box are conducted by using an eighth-order compact finite …

The geometric characteristics of dust clouds provide important information on the physical
processes that structure such clouds. One of such characteristics is the 2D fractal dimension …

It has recently been shown that turbulence in the interstellar medium can significantly
accelerate the growth of dust grains by accretion of molecules, but the turbulent gas density …

We study the linear growth and non-linear saturation of the 'acoustic Resonant Drag
Instability'(RDI) when the dust grains, which drive the instability, have a wide, continuous …

We investigate the dynamics of interstellar dust particles in moderately high resolution (5123
grid points) simulations of forced compressible transonic turbulence including self-gravity of …

Turbulence can significantly accelerate the growth of dust grains by accretion of molecules.
For dust dynamically coupled to the gas, the growth rate scales with the square of the Mach …

Planetesimals are believed to be formed by the coagulation of dust grains in the
protoplanetary disk turbulence. However, the bouncing and fragmentation barriers have not …