Physical and chemical conditions in methanol maser selected hot cores and UCH II regions

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Physical and chemical conditions in methanol maser selected hot cores and UCH II regions

We present the results of a targeted 3-mm spectral line survey towards the eighty-three 6.67GHz methanol maser selected star-forming clumps observed by Purcell. In addition to the previously reported measurements of HCO+(1-0), H13CO+(1-0) and CH3CN(5-4) and (6-5), we used the Mopra antenna to detect...

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Bibliographic Details
Main Authors:	Purcell, C., Longmore, S., Burton, M., Walsh, Andrew, Minier, V., Cunningham, M., Balasubramanyam, R.
Format:	Journal Article
Published:	Oxford University Press 2009
Subjects:	stars: pre-main-sequence ISM: molecules surveys ISM: abundances stars: formation
Online Access:	http://mnras.oxfordjournals.org/content/394/1/323.full.pdf+html http://hdl.handle.net/20.500.11937/21021

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