Studies of Molecular Clouds associated with H II Regions: S175
Mohaddesseh Azimlu, Michel Fich, Carolyn McCoey

TL;DR
This study investigates how HII regions influence nearby molecular clouds by analyzing their structure, physical properties, and turbulence, revealing contrasting effects on two condensations within the cloud.
Contribution
First detailed molecular line observations of S175, comparing two condensations to understand HII region impact on molecular cloud dynamics and star formation.
Findings
S175A is heated and compressed but remains quiescent.
S175B is turbulent and hosts an outflow.
HII regions can both trigger and suppress star formation.
Abstract
We are studying the impact of HII regions on star formation in their associated molecular clouds. In this paper we present JCMT RxA molecular line observations of S175 and environs. This is the first within a sample of ten HII regions and their surrounding molecular clouds selected for our study. We first make 7'x 7' maps in CO(2-1), which are used to investigate the structure of the cloud and to identify individual clumps. Single point observations were made in CO(2-1) and CS(5-4) at the peak of the CO(2-1) emission within each clump in order to measure the physical properties of the gas. Densities, temperatures, clump masses, peak velocities, and line widths were measured and calculated using these observations. We have identified two condensations (S175A and S175B) in the molecular cloud associated with this HII region. S175A is adjacent to the ionization front…
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