paper

The Effect of an Inert Solid Reservoir on Molecular Abundances in Dense Interstellar Clouds

arXiv:1301.1830 · doi:10.1515/astro-2017-0402

Abstract

The question, what is the role of freeze-out of chemical species in determining the molecular abundances in the interstellar gas is a matter of debate. We investigate a theoretical case of a dense interstellar molecular cloud core by time-dependent modelling of chemical kinetics, where grain surface reactions deliberately are not included. That means, the gas-phase and solid-phase abundances are influenced by gas reactions, accretion on grains, and desorption, only. We compare the results to a reference model, where no accretion occurs and only gas-phase reactions are included. We can trace that the purely physical processes of molecule accretion and desorption have major chemical consequences on the gas-phase chemistry. The main effect of introduction of the gas-grain interaction is long-term molecule abundance changes that come nowhere near an equilibrium in during the typical lifetime of a prestellar core.

8 pages, 6 figures, 1 table. Material initially presented in conference BAASP 2012 at Ventspils University College, May 2012

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