Compact dusty clouds and efficient H${}_2$ formation in diffuse ISM

Abstract

The formation of compact dusty clouds in diffuse interstellar medium (ISM) has been recently proposed and studied by Tsytovich et al. (2014). In the present paper, an effect of the clouds on the rate of H$\to$H${}_2$ transition in the ISM is examined. We discuss the mechanisms leading to the formation of the clouds and the creation of gaseous clumps around them, analyze the main processes determining the efficiency of the recombination of atomic hydrogen on dust grains, and estimate the expected enhancement of the global H${}_2$ formation due to the presence of the clouds. In conclusion, we argue that the compact dusty clouds provide optimum conditions for the atomic recombination in diffuse ISM, and point out some astrophysical implications of the resulting H${}_2$ formation enhancement.

5 pages, 2 figures, accepted to The Astrophysical Journal

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Cited by in corpus (2)

• Spatial distribution of Dust Density Wave Properties in Fluid Complex Plasmas
• Optical properties and dust temperatures in clumpy diffuse medium