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The Temperature Structure of Dusty Planetary Nebulae

Published online by Cambridge University Press:  26 May 2016

Graẓyna Stasińska  and
Ryszard Szczerba
Graẓyna Stasińska
Affiliation:
DAEC, Observatoire de Paris-Meudon, F-92195 Meudon Cedex, France
Ryszard Szczerba
Affiliation:
NCAC, Rabiańska 8, 87–100 Toruń, Poland

Abstract

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We have computed photoionization models of planetary nebulae containing dust. Photoelectric heating by small grains has an important effects on the temperature structure of the nebulae and could solve a number of problems that have found no satisfactory solution so far.

Type
Part V: Dust and Molecules in Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 308
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Dopita, M.A., & Sutherland, R.S. 2000, ApJ, 539, 742 Google Scholar
Liu, X.-W., Storey, P.J., Barlow, M.J., et al. 2000, MNRAS, 312, 585 Google Scholar
Peimbert, M., 1967, ApJ, 150, 825 Google Scholar
Stasińska, G., & Szczerba, R. 2001, A&A, 379, 1024 Google Scholar