Infrared Radiation of Planetary Nebulae

  • Grigor A. Gurzadyan
Part of the Astronomy and Astrophysics Library book series (AAL)

Abstract

The emission lines of gaseous nebula with wavelengths from 1 µm up to 100 µm are attributed to the infrared band. The corresponding composition and typical structure of the PN spectra is shown in Fig. 10.1.

Keywords

Dust Silicate Recombination Helium Reso 

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Copyright information

© Springer-Verlag Berlin Heidelberg 1997

Authors and Affiliations

  • Grigor A. Gurzadyan
    • 1
  1. 1.Garny Space Astronomy InstituteYerevan 2Armenia

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