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Experimental Measurements of Ion-Molecule Reactions

Published online by Cambridge University Press:  14 August 2015

F. C. Fehsenfeld
F. C. Fehsenfeld*
Affiliation:
NOAA/ERL, Aeronomy Laboratory, Boulder, Colorado 80303

Abstract

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The applicability of ion-molecule reaction rate constants measured at room temperature to simulation of interstellar cloud chemistry is discussed. Three-body association-rate constants of C+ and NH+3 have been measured between 100 K and 300 K. These results give information about the same associations by radiative processes. Possible implications for interstellar molecule production by radiative association and free radical reaction are discussed.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 291 - 296
Copyright
Copyright © Reidel 1980 

References

Albritton, D.L.: 1978, Atomic Data Nuclear Data Tables 22, 1-101.CrossRefGoogle Scholar
Black, J.H., and Dalgarno, A.: 1973, Astrophys. Lett. 15, 79.Google Scholar
Dotan, I., Fehsenfeld, F.C., and Albritton, D.L.: 1979, J. Chem. Phys. 71, 2728.CrossRefGoogle Scholar
Fehsenfeld, F.C., and Ferguson, E.E.: 1971, J. Geophys. Res. 76, 8453.CrossRefGoogle Scholar
Fehsenfeld, F.C., and Ferguson, E.E.: 1972, J. Chem. Phys. 56, 3077.CrossRefGoogle Scholar
Fehsenfeld, F.C., Lindinger, W., Schmeltekopf, A.L., Albritton, D.L., and Ferguson, E.E.: 1975, J. Chem. Phys. 62, 2001.CrossRefGoogle Scholar
Fehsenfeld, F.C.: 1976, Astrophys. J. 209, 638.CrossRefGoogle Scholar
Herbst, E.: 1976, Astrophys. J. 205, 94.CrossRefGoogle Scholar
Herbst, E.: 1977, Astrophys. J. 213, 696.CrossRefGoogle Scholar
Herbst, E.: 1979, Astro. and Space Sci. 65, 13.CrossRefGoogle Scholar
Herbst, E., and Klemperer, W.: 1973, Astrophys. J. 185, 505.CrossRefGoogle Scholar
Huntress, W.T.: 1977, Astrophys. J. 33, 495.CrossRefGoogle Scholar
Karpas, Z., Anicich, V., and Huntress, W.T.: 1979, J. Chem. Phys. 70, 2877.CrossRefGoogle Scholar
Prasad, S.S. and Huntress, W.T.: 1979a, Astrophys. J. Suppl. (accepted).Google Scholar
Prasad, S.S., and Huntress, W.T.: 1979b, Astrophys. J. (accepted).Google Scholar
Sieck, L.W.: 1979, SNRDS-NBS 64 (Washington, U.S. Government Printing Office).Google Scholar
Smith, D., and Adams, N.G.: 1979, Gas Phase Ion Chemistry, Vol. I, ed. Bowers, M.T., (Academic Press, New York) pp 1-44.Google Scholar
Townes, C.H.: 1977, Observatory, 97, 52.Google Scholar
Viggiano, A.A., Howorka, F., Albritton, D.L., Fehsenfeld, F.C., Adams, N.G., and Smith, D.: 1979, Astrophys. J., (to be submitted).Google Scholar
Watson, W.P.: 1974, Astrophys. J. 188, 35.CrossRefGoogle Scholar
Woodin, R.L., and Beauchamp, J.L.: 1978, J. Amer. Chem. Soc. 78, 502.Google Scholar