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dc.creatorLinnartz, H.en_US
dc.creatorMotylewski, T.en_US
dc.creatorMaier, John P.en_US
dc.date.accessioned2006-06-15T19:01:36Z
dc.date.available2006-06-15T19:01:36Z
dc.date.issued1998en_US
dc.identifier1998-MI-03en_US
dc.identifier.urihttp://hdl.handle.net/1811/18841
dc.descriptionAuthor Institution: Institute for physical chemistry, University of Baselen_US
dc.description.abstractA rotationally resolved spectrum of the $^{2}\Pi-X^{2}\Pi$ electronic transition of $C_{6}H$ and $C_{6}D$ in the gas phase is presented, using cavity ring down spectroscopy in combination with a supersonic slit nozzle discharge technique. The source offers the possibility to generate a dense and cold $(T_{rot} < 25 K)$ carbon plasma that is stable for many hours. Both the experiment and the first results, aimed at locating the electronic transitions of neutral carbon chains of possible astrophysical interest, will be presented.en_US
dc.format.extent72941 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleCAVITY RING DOWN SPECTROSCOPY IN A PULSED SUPERSONIC SLIT NOZZLE DISCHARGEen_US
dc.typearticleen_US


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