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The Distribution of Molecular Hydrogen in Planetary Nebulae

Published online by Cambridge University Press:  04 August 2017

J. W. V. Storey ,
B. L. Webster ,
P. Payne  and
M. A. Dopita
J. W. V. Storey
Affiliation:
School of Physics, University of New South Wales Kensington, Australia
B. L. Webster
Affiliation:
School of Physics, University of New South Wales Kensington, Australia
P. Payne
Affiliation:
School of Physics, University of New South Wales Kensington, Australia
M. A. Dopita
Affiliation:
Mt. Stromlo & Siding Spring Observatory Canberra, Australia

Abstract

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A correlation has been found between strong molecular hydrogen emission and the morphological type of a planetary nebula. Those with an equatorial toroid and bipolar extensions have H2 1−0 S(1) stronger than Brackett γ. H2 maps of several objects, and NGC 2346 in particular, are consistent with a fast stellar wind interacting with an anisotropic medium.

Type
Circumstellar Shells
Information
Symposium - International Astronomical Union , Volume 120: Astrochemistry , 1987 , pp. 339 - 340
Copyright
Copyright © Reidel 1987 

References

1. Beckwith, S., 1978. Calif. Int. Tech. Google Scholar
2. Beckwith, S., Persson, S.E. & Gatley, I., 1978. Astrophys. J., 219, L33.CrossRefGoogle Scholar
3. Issacman, R., 1984. Astr. Astrophys., 130, 151.Google Scholar
4. Phillips, J.P., Reay, N.K. & White, G.J., 1983. Mon. Not. Roy. Astr. Soc., 193, 977.CrossRefGoogle Scholar
5. Phillips, J.P., White, G.J. & Harten, R., 1985. Astron. Astrophys., 145, 118.Google Scholar
6. Storey, J.W.V., 1984. Mon. Not. Roy. Astr. Soc., 206, 521.CrossRefGoogle Scholar
7. Treffers, R.T., Fink, U.F., Larson, P.L. & Gautier, N.T., 1976, Ap. J., 209, 793.CrossRefGoogle Scholar
8. Present paper.Google Scholar