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dc.creatorWatson, William D.en_US
dc.creatorWyld, H. W.en_US
dc.date.accessioned2008-01-12T13:40:45Z
dc.date.available2008-01-12T13:40:45Z
dc.date.issued2007en_US
dc.identifier2007-RD-10en_US
dc.identifier.urihttp://hdl.handle.net/1811/31248
dc.descriptionAuthor Institution: Department of Physics,University of Illinois, Urbana,; IL 61801en_US
dc.description.abstractCalculational methods and results will be presented for the emergent maser radiation from a thin, gaseous disk undergoing Keplerian rotation. The parameters that describe the masing and the disk are intended to reflect those of disks around young stars. Saturation by the maser radiation--which is likely to be present-- has not previously been incorporated into such calculations in astronomy. Saturation causes the velocity distribution of excited, masing molecules to deviate from Maxwellian (``hole burning") and greatly increases the calculational challenge. Comparisons will be made with observational data.en_US
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleSATURATED MASER RADIATION FROM A CIRCUMSTELLAR, KEPLERIAN DISKen_US
dc.typearticleen_US


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