Infrared Radiation of Planetary Nebulae

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


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.


Emission Line Dust Particle Electron Temperature Infrared Radiation Infrared Emission 
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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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