Understanding the physics of turbulence is crucial for many applications, including weather,
industry and astrophysics. In the interstellar medium,, supersonic turbulence plays a crucial …

Turbulent diffusion flames are considered an active field of research used in many
engineering applications of combustion theory. The basic properties of jet diffusion flames …

The presence of Galactic cirrus is an obstacle for studying both faint objects in our Galaxy
and low surface brightness extragalactic structures. With the aim of studying individual cirrus …

Shocks form the basis of our understanding for the density and velocity statistics of
supersonic turbulent flows, such as those found in the cool interstellar medium (ISM). The …

We develop an analytic model for the power spectra of polarized filamentary structures as a
way to study the Galactic polarization foreground to the cosmic microwave background. Our …

Stars form in highly magnetized, supersonic turbulent molecular clouds. Many of the tools
and models that we use to carry out star formation studies rely upon the assumption of cloud …

Complex turbulent motions of magnetized gas are ubiquitous in the interstellar medium
(ISM). The source of this turbulence, however, is still poorly understood. Previous work …

Supersonic turbulence is a key player in controlling the structure and star formation potential
of molecular clouds (MCs). The three-dimensional (3D) turbulent Mach number,, allows us to …

Different studies have reported a power-law mass–size relation M∝ R q for ensembles of
molecular clouds. In the case of nearby clouds, the index of the power-law q is close to 2 …

It is well known that departure from sphericity in the geometry of primordial dark matter halos
modifies their mass function. The ellipsoidal collapse model yields a better agreement with …