THE MILLIMETER - AND SUBMILLIMETER - WAVE SPECTRUM OF METHYL FORMATE $(HCOOCH_{3})$ AND SYMMETRIC MONODEUTERATED METHYL FORMATE $(DCOOCH_{3})$
dc.creator | Oesterling, L. C. | en_US |
dc.creator | Ferguson, D. W. | en_US |
dc.creator | Herbst, E. | en_US |
dc.creator | De Lucia, Frank C. | en_US |
dc.date.accessioned | 2007-11-20T17:14:52Z | |
dc.date.available | 2007-11-20T17:14:52Z | |
dc.date.issued | 1995 | en_US |
dc.identifier | 1995-TK-07 | en_US |
dc.identifier.uri | http://hdl.handle.net/1811/29869 | |
dc.description | Author Institution: The Ohio State University, 174 West 18th Avenue, Columbus, OH 43210. | en_US |
dc.description.abstract | Although deuterated isotopomers of organic molecules have been detected in various interstellar sources, singly deuterated isotopomers have not yet been detected in the interstellar medium due to a lack of laboratory spectroscopic data. To aid in the study of interstellar spectra, the analysis of the rotational-torsional spectrum of deuterated $methy^{l}$ formate has been extended into the millimeter-wave and submillimeter-wave regions of the electromagnetic spectrum. The A (symmetric) and E (asymmetric) torsional substates of the ground $(\nu_{t} = 0)$ torsional state of deuterated methyl formate have been fit to a rms deviation of 85 kHz using a direct digonalization procedure of an extended global internal -axis method (IAM) Hamiltonian. Using this global IAM approach, the A and E states of the ground torsional state for methyl formate have been reanalyzed and a rms deviation of less than 100 kHz has been obtained for the global fit of our data. | en_US |
dc.format.extent | 53011 bytes | |
dc.format.mimetype | image/jpeg | |
dc.language.iso | English | en_US |
dc.publisher | Ohio State University | en_US |
dc.title | THE MILLIMETER - AND SUBMILLIMETER - WAVE SPECTRUM OF METHYL FORMATE $(HCOOCH_{3})$ AND SYMMETRIC MONODEUTERATED METHYL FORMATE $(DCOOCH_{3})$ | en_US |
dc.type | article | en_US |
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