Klemperer, William

Kitaura Kazuo, 804 Klein Douglas J., 173 Klein Oskar, 123 Klemperer William, 3 Klinowski Jacek, XXXIII Kobus Jacek, 432 Koch Wolfram, 676, 715... 

Alice P. Gast, Massachusetts Institute of Technology, Co-Chair William Klemperer, Harvard University, Co-Chair Arthur I. Bienenstock, Stanford University A. Welford Castleman, Jr., The Pennsylvania State University Andrea W. Chow, Caliper Technologies Corp. 

William Klemperer, Department of Chemistry, Harvard University, Cambridge, Massachusetts, USA... 

FHL wishes to thank Professor William Klemperer at Harvard University for his encouragement and guidance. The authors thank Robert A. Forbes for his suggestions and for reading the manuscript. Finally the authors are grateful to Michelle V. Buchanan for her tremendous efforts in organizing this FTMS book. 

The most important process for the formation of the initial polyatomic species is radiative association. Upon collision, a large unstable molecule in an excited state ( collisional complex ) may form, which is stabilized with a low probability by the emission of a photon (e.g. Bates 1951 Williams 1972 Herbst Klemperer 1973). For example, the formation of light hydrocarbons starts with radiative association of C+ and H2, leading to excited CH ( o = 4.0 10-16 cm-3 s-1 and = —0.2, Herbst 1985). Despite their importance, rates of many radiative association processes remain unknown because they are difficult to measure in the laboratory or predict theoretically (Herbst Dunbar 1991). 

FIGURE 3-3 IR spectrum of A -methylacetamide in various solvents in the N—H stretching region 0.4 M at 30 G. [Unpublished spectra of William A. Klemperer and George C. Pimentel]... 

Department of Theology, Georgetown University, Washington, D.C. 20057, USA William Klemperer... 

Joseph M. Desimone, University of North Carolina, Chapel Hill, and North Carolina State University Catherine Fenselau, University of Maryland Jon Franklin, University of Maryland Richard M. Gross, Dow Chemical Company Nancy B. Jackson, Sandia National Laboratory Sangtae Kim, Eli Lilly and Company William Klemperer, Harvard University Thomas J. Meyer, Los Alamos National Laboratory Paul J. Reider, Amgen, Inc. 

Robert Field thanks Richard F. Barrow, Thomas H. Bergeman, Padraic Burns, Daniel Cossart, Stephen L. Coy, F. Fleming Crim, Matthew P. Jacobson, Caroline C. Jarrold, David M. Jonas, Christian Jungen, Aposto-los Kalemos, Michael E. Kellman, James L. Kinsey, William Klemperer, Roland Lefebvre, Robert H. Lipson, Anthony J. Merer, Frederic Merkt, David C. Oertel, Stephen T. Pratt, Joelle and Frangois Rostas, Robert J. Silbey, Adam H. Steeves, Patrick H. Vaccaro, and James K. G. Wat-... 

Persei, confirmed by the Copernicus satellite in 1973. The matter in the space dust furnishes the third body required for reaction, hence the finding of H2 in such clouds. Carruthers, an African American, invented the FUV camera-spectrograph carried to the Moon on Apollo 16 in 1972. Hydrogen (H2) is the most abundant molecule in space. Tbe second most abundant molecule, carbon monoxide (CO), was discovered in 1970 at levels one 10-thousandth those of H2. William Klemperer (1927- ) at Harvard has noted that the reaction ... 

Balocchi FA, Williams JH, Klemperer W (1983) Moleculm betun studies of CeFe, C6F3H3, and CeHs complexes of HR The rotational spectrum of CeHe-HF. J Phys Chem 87 2079-2084... 

William Klemperer, David Yaron, and David D. Nelson Jr. Faraday Discuss. Chem. Soc., 86 261, 1988. 

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