Hostname: page-component-788cddb947-tr9hg Total loading time: 0 Render date: 2024-10-14T05:14:37.706Z Has data issue: false hasContentIssue false
  • English
  • Français

Recombination Processes

Published online by Cambridge University Press:  18 September 2017

P. J. Storey
P. J. Storey*
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, LONDON WC1E 6BT, England

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The role of resonances in the photoionization cross-sections of ions is discussed in relation to the radiative recombination coefficient. The calculation of dielectronic contributions to the recombination coefficient is reviewed for nebular conditions, and the importance of autoionizing states close to the first ionization threshold is illustrated. For those ions for which dielectronic recombination is not important at nebular temperatures, an assessment of the accuracy of the best available recombination coefficients is given.

Type
Section II: Physical Processes in Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 103: Planetary Nebulae , 1983 , pp. 199 - 209
Copyright
Copyright © Reidel 1983 

References

Aldrovandi, S.M.V. and Péquignot, D., 1973. Astron. Astrophys., 25, 137.Google Scholar
Aldrovandi, S.M.V. and Péquignot, D., 1974. Rev. Bras, de Fis., 4, no 3, 491.Google Scholar
Aldrovandi, S.M.V. and Péquignot, D., 1976. Astron. Astrophys., 47, 321.Google Scholar
Baker, J.G. and Menzel, D.H., 1938. Astrophys. J., 88, 52.Google Scholar
Beigman, I.L. and Chichkov, B.N., 1980. J. Phys. B., 13, 565.Google Scholar
Brocklehurst, M., 1970. Mon. Not. R. astr. Soc., 148, 417.Google Scholar
Brocklehurst, M., 1971. Mon. Not. R. astr. Soc., 153, 471.Google Scholar
Brocklehurst, M., 1972. Mon. Not. R. astr. Soc., 157, 211.Google Scholar
Burgess, A., 1964. Astrophys. J., 139, 776.Google Scholar
Burgess, A., 1965. Astrophys. J., 141, 1588.Google Scholar
Davies, P.C.W. and Seaton, M.J., 1969. J. Phys. B., 2, 757.Google Scholar
Davis, J., Jacobs, V.L., Kepple, P.C. and Blaha, M., 1977. J. Quant. Spectrosc. Radiat. Transfer, 17, 139.Google Scholar
Giles, K., 1977. Mon. Not. R. astr. Soc., 180, 57P.Google Scholar
Gould, R.J., 1978. Astrophys. J., 219, 250.Google Scholar
Jacobs, V.L., Davis, J., Kepple, P.C. and Blaha, M., 1977. Astrophys. J., 215, 690.Google Scholar
Jacobs, V.L., Davis, J., Rogerson, J.E. and Blaha, M., 1979. Astrophys. J., 230, 627.Google Scholar
Jacobs, V.L., Davis, J., Rogerson, J.E., Blaha, M., Cain, J. and Davis, M., 1980. Astrophys. J., 239, 1119.Google Scholar
Nussbaumer, H. and Storey, P.J., 1983. Astron. Astrophys., to be submitted.Google Scholar
Seaton, M.J., 1978. Mon. Not. R. astr. Soc., 185, 5P.Google Scholar
Seaton, M.J., 1980. “Radio Recombination Lines”, ed. Shaver, P.A. (D. Reidel),3.Google Scholar
Seaton, M.J. and Storey, P.J., 1976. “Atomic Processes and Applications”, ed. Burke, P.G. and Moiseiwitsch, B.L. (North-Holland), chapter 6.Google Scholar
Shull, M.J. and Van Steenberg, M., 1982. Astrophys. J. Suppl., 48, 95.Google Scholar
Storey, P.J., 1981. Mon. Not. R. astr. Soc., 195, 27P.Google Scholar
Summers, H.P., 1974. Appleton Laboratory, IM 367.Google Scholar
Weisheit, J. and Walmsley, C.M., 1977. Astron. Astrophys., 61, 141.Google Scholar