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dc.creatorFriedel, Douglas N.en_US
dc.date.accessioned2013-07-16T21:33:52Z
dc.date.available2013-07-16T21:33:52Z
dc.date.issued2013en_US
dc.identifier2013-RF-05en_US
dc.identifier.urihttp://hdl.handle.net/1811/55201
dc.descriptionAuthor Institution: Department of Astronomy, University of Illinois, 1002 W. Green St., Urbana, IL 61801en_US
dc.description.abstractAfter our successful molecular studies of the high mass star forming region Orion-KL (Friedel \& Widicus Weaver 2012, ApJS, 201, 17; Widicus Weaver \& Friedel 2012, ApJS, 201, 16) we have observed three more high mass star forming regions (W3, W75N, and W51). The purpose of these observations is to further constrain the physical conditions under which the different complex organic molecules form and survive. The results of these observations as well as their impact on current molecular formation models will be presented.en_US
dc.language.isoenen_US
dc.publisherOhio State Universityen_US
dc.titleMULTI-RESOLUTION STUDIES OF COMPLEX MOLECULES IN HIGH MASS STAR FORMING REGIONSen_US
dc.typeArticleen_US


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