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dc.creatorChen, Weien_US
dc.creatorMcCarthy, M. C.en_US
dc.creatorTravers, Michael J.en_US
dc.creatorThaddeus, P.en_US
dc.creatorGottlieb, Elaine W.en_US
dc.creatorGottlieb, C. A.en_US
dc.creatorMunrow, Michaeleen R.en_US
dc.creatorNovick, Stewart E.en_US
dc.date.accessioned2006-06-15T15:41:29Z
dc.date.available2006-06-15T15:41:29Z
dc.date.issued1997en_US
dc.identifier1997-MI-09en_US
dc.identifier.urihttp://hdl.handle.net/1811/13887
dc.descriptionAuthor Institution: Harvard-Smithsonia Center for Astrophysics; Division of Applied Sciences, Harvard University; Department of Chemistry, Wesleyan Universityen_US
dc.description.abstractThe cyanomethyl radical, $H_{2} CCN$, was first found in the interstellar medium and then detected in the laboratory in 1988, however, the longer members of this sequence have remained undetected. We report the first detection of the cyanopropynyl radical, $H_{2} CCCCN$, in a pulsed-discharge nozzle Fourier transform microwave spectrometer. Four rotational transitions (N=2-1 through 5-4) of both $H_{2} CCCCN$ and $H_{2}CCCC^{15}N$ were measured and the complex fine and hyperfine structure was assigned. These results will be presented and the possibility of detecting the next member of the series will be discussed.en_US
dc.format.extent110246 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleLABORATORY DETECTION OF THE NEW CARBON CHAIN RADICAL $H_{2}CCCCN$en_US
dc.typearticleen_US


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