most citedStatistical link between the structure of molecular clouds and their density distribution

17 citations · 17 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2024

Multiple power-law tails in the density and column-density distribution in contracting star-forming clumps

Todor V. Veltchev, Philipp Girichidis, Lyubov Marinkova +3

We present a numerical study of the evolution of power-law tails (PLTs) in the (column-)density distributions (-PDF, -PDF) in contracting star-forming clumps in primordial ga…

astro-ph.GA2023

Thermodynamics of fluid elements in the context of saturated isothermal turbulence in molecular clouds

Sava Donkov, Ivan Zh. Stefanov, Todor V. Veltchev

The presented paper is an attempt to investigate the dynamical states of an hydrodynamical isothermal turbulent self-gravitating system using some powerful tools of the classical t…

physics.ed-ph2023

Isochoric cooling of air in the University Physics laboratory

Ivan Z. Stefanov, Sava Donkov, Nikolay Denev

In this paper an alternative way of conducting the physics laboratory exercise for determining the adiabatic index of air using the Clement -- Desormes method is proposed. The proc…

physics.ed-ph2023

Video analysis of the damped oscillations of Pohl's pendulum

Ivan Z. Stefanov, Nikolay Denev, Sava Donkov

In this paper problems that arose with the introduction of distance learning in physics at the Technical University of Sofia due to the COVID-19 pandemic and the imposition of vide…

astro-ph.GA201617 cited

Statistical link between the structure of molecular clouds and their density distribution

Sava Donkov, Todor V. Veltchev, Ralf S. Klessen

We introduce the concept of a class of equivalence of molecular clouds represented by an abstract spherically symmetric, isotropic object. This object is described by use of abstra…

astro-ph.SR2012

Modeling of molecular clouds with formation of prestellar cores

Sava Donkov, Orlin Stanchev, Todor V. Veltchev

We develop a statistical approach for description of dense structures (cores) in molecular clouds that might be progenitors of stars. Our basic assumptions are a core mass-density…