activity
20112020
most citedModel of the vibrationally excited HO maser at 658 GHz in circumstellar envelopes around asymptotic giant branch stars

11 citations · 18 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2020

Collisional Pumping of OH Masers near Supernova Remnants

A. V. Nesterenok

The collisional pumping of OH masers in non-dissociative C-type shocks near supernova remnants is considered. The emergence of maser emission in OH lines is investigated for variou…

astro-ph.GA2020

The Sobolev approximation for radiation transport with line overlap and continuous opacity

Aleksandr Nesterenok

The radiation transport problem in the plane-parallel medium with the large velocity gradient is considered. The Sobolev approximation is used. The effects of continuum absorption…

astro-ph.GA2019

Chemical evolution of cold dark clouds in the vicinity of supernova remnants

A. V. Nesterenok

The supernova explosion increases cosmic ray and x-ray fluxes in the surrounding interstellar medium. Cosmic ray particles and x-ray radiation penetrate nearby molecular clouds and…

astro-ph.GA2019

C-type shock modelling -- the effect of new H-H collisional rate coefficients

A. V. Nesterenok, D. Bossion, Y. Scribano +1

We consider collisional excitation of H molecules in C-type shocks propagating in dense molecular clouds. New data on collisional rate coefficients for (de-)excitation of H

astro-ph.GA2018

Chemical evolution of the gas in C-type shocks in dark clouds

A. V. Nesterenok

A magnetohydrodynamic model of a steady, transverse C-type shock in a dense molecular cloud is presented. A complete gas-grain chemical network is taken into account: the gas-phase…

astro-ph.SR201511 cited

Model of the vibrationally excited HO maser at 658 GHz in circumstellar envelopes around asymptotic giant branch stars

Aleksandr Nesterenok

The model is presented of HO maser in the line within the first excited vibrational state of the molecule around oxygen-rich asymptotic giant branch stars. It i…