HC3N mapping observations toward massive star-forming cores

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Galactic, Mopra

Scientific paper

We propose to do high resolution OTF mapping observations with HC3N(12-11 and 10-9) and other species relevant to the formation mechanism of HC3N toward four massive star-forming regions. With the multiple-line mapping, we can expect to find the distribution of high velocity components as well as the chemistry of HC3N, and can give some clues of the chemical evolution of massive star formation.

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