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arXiv · 1908.05394

Molecular envelope around the HII region RCW 120

M. S. Kirsanova·Ya N. Pavlyuchenkov·D. S. Wiebe·P. A. Boley·S. V. Salii·S. V. Kalenskii·A. M. Sobolev·L. D Anderson
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Abstract

The H II region RCW120 is a well-known object, which is often considered as a target to verify theoretical models of gas and dust dynamics in the interstellar medium. However, the exact geometry of RCW120 is still a matter of debate. In this work, we analyse observational data on molecular emission in RCW120 and show that 13CO(2-1) and C18O(2-1) lines are fitted by a 2D model representing a ring-like face-on structure. The changing of the C18O(3-2) line profile from double-peaked to single-peaked from the dense molecular Condensation 1 might be a signature of stalled expansion in this direction. In order to explain a self-absorption dip of the 13CO(2-1) and 13CO(3-2) lines, we suggest that RCW120 is surrounded by a diffuse molecular cloud, and find confirmation of this cloud on a map of interstellar extinction. Optically thick 13CO(2-1) emission and the infrared 8 um PAH band form a neutral envelope of the H II region resembling a ring, while the envelope breaks into separate clumps on images made with optically thin C18O(2-1) line and far-infrared dust emission.

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M. S. Kirsanova, Ya N. Pavlyuchenkov, D. S. Wiebe, P. A. Boley, S. V. Salii, S. V. Kalenskii, A. M. Sobolev, L. D Anderson. 2019-08-15. Molecular envelope around the HII region RCW 120. https://doi.org/10.1093/mnras/stz2048

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