Skip to main content
Log in

On the effect of collisional ionization during the time evolution of Hii regions

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

The set of equations describing the time evolution ofHii regions, accounting for collisional ionization, are presented. Differential forms of these equations are deduced, and it is shown that it is not necessary within this context to consider changes in the potential energy due to ionization of the gas.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Axford, W. I.: 1961,Phil. Trans. Roy. Soc. London,A253, 201.

    Google Scholar 

  • Goldsworthy, F. A.: 1961,Phil. Trans. Roy. Soc. London,A253, 277.

    Google Scholar 

  • Kahn, F. D.: 1954,Bull. Astron. Inst. Netherlands 12, 456, 187.

    Google Scholar 

  • Mathews, W. G.: 1965,Astrophys. J. 142, 1120.

    Google Scholar 

  • Woolley, R. R. and Stibbs, D. W.: 1953,The Outer Layers of a Star, Oxford, Clarendon Press.

    Google Scholar 

  • Zel'dovich, Ya. B. and Raizer, Yu. P.: 1967,Physics of Shock Waves and High Temperature Hydrodynamic Phenomena, Academic Press, New York and London.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Tenorio-Tagle, G. On the effect of collisional ionization during the time evolution of Hii regions. Astrophys Space Sci 47, 225–228 (1977). https://doi.org/10.1007/BF00651369

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00651369

Keywords

Navigation