dc.creator Maillard, J.- P. en_US dc.creator Chauville, J. en_US dc.creator Mantz, A. W. en_US dc.date.accessioned 2006-06-15T13:51:38Z dc.date.available 2006-06-15T13:51:38Z dc.date.issued 1976 en_US dc.identifier 1976-WA-7 en_US dc.identifier.uri http://hdl.handle.net/1811/9916 dc.description This research was supported by the National Research Council of Canada through Grant No. A6025. Permanent address of R. H. Tipping: Department of Physics, Memorial University of Newfoundland, St. John's, Newfoundland, Canada, A1C 5S7 en_US dc.description Author Institution: Observatoire de Meudon, Laboratoire du Telescope Infrarouge; Observatoire de Meudon, Digilab, Inc. en_US dc.description.abstract The vibration-rotation OH spectrum emitted by an acetylene oxygen flame has been measured between 2700 and $11 000 cm^{-1}$ with a high resolution Fourier Spectrometer. The main interferences in the spectra are due to water vapor absorption and emission necessarily mixed with OH in the source. Nevertheless, line positions to high J values (more than 20 for some P branches) of the 1-0, 2-1 bands of the $\Delta v = 1$ sequence, 2-0, 3-1, 4-2, 5-3 of ${\Delta} v$ = 2 and 3-0, 4-1, 5-2 bands of ${\Delta} v = 3$ are reported. Molecular constants for each band were derived by using a computer program described by Albritton, et al. Ground state molecular constants of OH were derived from a least squares fit to these data, weighted according to their estimated uncertainties. Uncertainties in the molecular constants derived from these data are considerably improved relative to the previously available constants. Predicted positions of some unobserved bands of OH have been determined from these new constants for the purpose of aiding stellar atmospheric studies. en_US dc.format.extent 141881 bytes dc.format.mimetype image/jpeg dc.language.iso English en_US dc.publisher Ohio State University en_US dc.title HIGH RESOLUTION EMISSION SPECTRUM OF OH IN AN OXYACETYLENE FLAME FROM 3.7 TO 0.9 MICRONS. en_US dc.type article en_US
﻿

### Files in this item

Items in Knowledge Bank are protected by copyright, with all rights reserved, unless otherwise indicated.