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Hydrocarbons in Massive Star Forming Regions: C2H Observations
Published online by Cambridge University Press: 12 September 2016
Abstract
In order to better understand the chemical conditions and evolutionary properties of massive star-forming regions, and to explore the physical and chemical behavior of simple hydrocarbon molecules, we have used telescopes such as CSO, JCMT, CARMA and SMA, to map the multi-transitions of C2H and HC3N. The column densities and abundances are compared with chemical models to gain some diagnostic of the environment of the regions.
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- Copyright © International Astronomical Union 2016