activity
20032021
most citedModelling the optical properties of composite and porous interstellar grains

92 citations · 229 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2021★ 9 cited

Evolution of dust grain size distribution and grain porosity in galaxies

Hiroyuki Hirashita, Vladimir B. Il'in

The radiative properties of interstellar dust are affected not only by the grain size distribution but also by the grain porosity. We develop a model for the evolution of size-depe…

astro-ph.GA2021★ 15 cited

Fractal dimension of optical cirrus in Stripe82

Alexander A. Marchuk, Anton A. Smirnov, Aleksandr V. Mosenkov +4

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

astro-ph.GA2021★ 15 cited

Isochrone fitting of Galactic globular clusters -- III. NGC\,288, NGC\,362, and NGC\,6218 (M12)

George A. Gontcharov, Maxim Yu. Khovritchev, Aleksandr V. Mosenkov +6

We present new isochrone fits to colour-magnitude diagrams of the Galactic globular clusters NGC\,288, NGC\,362, and NGC\,6218 (M12). We utilize a lot of photometric bands from the…

astro-ph.GA2021★ 17 cited

Evolution of dust porosity through coagulation and shattering in the interstellar medium

Hiroyuki Hirashita, Vladimir B. Il'in, Laurent Pagani +1

The properties of interstellar grains, such as grain size distribution and grain porosity, are affected by interstellar processing, in particular, coagulation and shattering, which…

astro-ph.GA2017★ 13 cited

Mid-infrared extinction and fresh silicate dust towards the Galactic Center

Nikolai V. Voshchinnikov, Thomas Henning, Vladimir B. Il'in

We interpret the interstellar extinction observed towards the Galactic Center (GC) in the wavelength range $λ= 1 - 20\,\mkm$. Its main feature is the flat extinction at $3 - 8\,\mk…

astro-ph.GA2015★ 28 cited

Polarizing efficiency as a guide of grain growth and interstellar magnetic field properties

N. V. Voshchinnikov, V. B. Il'in, H. K. Das

We interpret the relation between the polarizing efficiency and the wavelength of the maximum polarization observed for 17 objects (including 243 stars…