Hostname: page-component-77c89778f8-n9wrp Total loading time: 0 Render date: 2024-07-24T05:33:44.346Z Has data issue: false hasContentIssue false

The Temperature Structure of Dusty Planetary Nebulae

Published online by Cambridge University Press:  26 May 2016

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

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.

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
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