We review recent advances in the analytical and numerical modeling of the star formation
rate in molecular clouds and discuss the available observational constraints. We focus on …

A large number of studies have found that the dark matter surface density, given by the
product of the dark matter core radius (rc) and core density (ρ c) is approximately constant …

We have investigated the shape of the extinction curve in the infrared up to~ 25μm for the
Orion A star-forming complex. The basis of this work is near-infrared data acquired with the …

Context. The properties of dust grains, in particular their size distribution, are expected to
differ from the interstellar medium to the high-density regions within molecular clouds. Aims …

Context. Quickly growing computing facilities and an increasing number of extragalactic
observations encourage the application of data-driven approaches to uncover hidden …

A large number of studies have found that the dark matter surface density, given by the
product of the dark matter core radius ($ r_c $) and core density ($\rho_c $) is approximately …

Radiation feedback from stellar clusters is expected to play a key role in setting the rate and
efficiency of star formation in giant molecular clouds (GMCs) and across whole galaxies. In …

In this paper we analyze the models of piecewise linear regression and its application for
solving the problem of approximation. We discuss the algorithm for finding the linear models …