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

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

Internet

http://mnras.oxfordjournals.org/content/394/1/323.full.pdf+html
http://hdl.handle.net/20.500.11937/21021

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