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dc.creatorO'Brien, L. C.en_US
dc.creatorLambeth, Amandaen_US
dc.date.accessioned2006-06-15T20:17:26Z
dc.date.available2006-06-15T20:17:26Z
dc.date.issued2001en_US
dc.identifier2001-WG-02en_US
dc.identifier.urihttp://hdl.handle.net/1811/20300
dc.descriptionAuthor Institution: Southern Illinois University; Department of Chemistry, Southern Illinois Universityen_US
dc.description.abstractThe near infrared electronic transition of CuSe has been observed for the first time. The spectrum of the $Y^{2}\Sigma^{+} - X^{2}\Pi$ transition, labeled by analogy with the CuO and CuS near infrared electronic transitions, was recorded with the Fourier transform spectrometer associated with the McMath-Pierce Solar Telescope, Kitt Peak, AZ. The CuSe molecules were produced in a King-type carbon tube furnace operating at 1800 C and at a total pressure of approximately 400 torr. The electronic term energy and vibrational constants for both states will be presented.en_US
dc.format.extent224513 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleTHE NEAR INFRARED $Y^{2}\Sigma^{+} - X^{2}\Pi$ TRANSITION OF COPPER SELENIDEen_US
dc.typearticleen_US


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