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Radiative Transfer Problems in Planetary Nebulae

Published online by Cambridge University Press:  18 September 2017

David G. Hummer
David G. Hummer*
Affiliation:
Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards, Boulder, Colorado, 80309

Extract

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In view of the enormous importance of the UV observations of planetary nebulae made possible by the IUE, this review will concentrate primarily on the formation of resonance lines in nebulae; an important special case is that of He II Lyα and its role in the Bowen mechanism. Special attention is given to the effects of dust on the line and continuum formation.

Type
Section II: Physical Processes in Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 103: Planetary Nebulae , 1983 , pp. 211 - 218
Copyright
Copyright © Reidel 1983 

References

Adams, T.F.: 1975, Astrophys. J. 201, pp. 350–351.Google Scholar
Bonilha, J.R.M., Ferch, R., Salpeter, E.E., and Slater, G.: 1979, Astrophys. J. 233, pp. 649–660.CrossRefGoogle Scholar
Flower, D.R. and Perinotto, M.: 1980, Mon. Not. R. astr. Soc. 191, pp. 301–308.Google Scholar
Frisch, H.: 1980, Astron. Astrophys. 87, pp. 357–360 Google Scholar
Grachev, S.I.: 1976, Vestn. Leningrad Gos. Univ., No. 1, pp. 128–132.Google Scholar
Grachev, S.I.: 1977a, Astrophysics 13, pp. 95–101.Google Scholar
Grachev, S.I.: 1977b, Vestn. Leningrad Gos. Univ., No. 19, pp. 114–120.Google Scholar
Grachev, S.I.: 1978a, Vestn. Leningrad Gos. Univ., No. 1, pp. 129–135.Google Scholar
Grachev, S.I.: 1978b, Astrophysics 14, pp. 63–69.CrossRefGoogle Scholar
Harrington, J.P.: 1972, Astrophys. J. 176, pp. 127–137.Google Scholar
Harrington, J.P.: 1973, Mon. Not. R. astr. Soc. 162, pp. 43–52.CrossRefGoogle Scholar
Harrington, J.P., Seaton, M.J., Adams, S., and Lutz, J.H.: 1982, Mon. Not. R. astr. Soc. 199, pp. 517–564.Google Scholar
Hummer, D.G. and Kunasz, P.B.: 1980, Astrophys. J. 236, pp. 609–618.Google Scholar
Hummer, D.G. and Rybicki, G.B.: 1971, Mon. Not. R. astr. Soc. 152, pp. 1–19.Google Scholar
Hummer, D.G. and Rybicki, G.B.: 1982a, Astrophys. J. 254, pp. 767–779.Google Scholar
Hummer, D.G. and Rybicki, G.B.: 1982b, Astrophys. J., in press.Google Scholar
Hummer, D.G. and Seaton, M.J.: 1963, Mon. Not. R. astr. Soc. 125, pp. 437–459.Google Scholar
Kallman, T. and McCray, R.A.: 1980, Astrophys. J. 242, pp. 615–627.Google Scholar
Kunasz, P.B. and Hummer, D.G.: 1974, Mon. Not. R. astr. Soc. 166, pp. 19–55.Google Scholar
Kneer, F.: 1975, Astrophys. J. 200, pp. 367–368.CrossRefGoogle Scholar
Leung, C.M.: 1975, Astrophys. J. 199, pp. 340–360.Google Scholar
Petrosian, V. and Dana, R.A.: 1980, Astrophys. J. 241, pp. 1094–1106.Google Scholar
Saraph, H.E. and Seaton, M.J.: 1980, Mon. Not. R. astr. Soc. 193, pp. 617–629.CrossRefGoogle Scholar
Van Blerkom, D. and Hummer, D.G.: 1967, Mon. Not. R. astr. Soc. 137, 353–374.Google Scholar
Weymann, R.J. and Williams, R.E.: 1969, Astrophys. J. 157, pp. 1201–1213.Google Scholar
Zanstra, H.: 1951, B.A.N. 11, pp. 341–358.Google Scholar