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.
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© 1997 Springer-Verlag Berlin Heidelberg
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Gurzadyan, G.A. (1997). Infrared Radiation of Planetary Nebulae. In: The Physics and Dynamics of Planetary Nebulae. Astronomy and Astrophysics Library. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-03448-4_10
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DOI: https://doi.org/10.1007/978-3-662-03448-4_10
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-08245-0
Online ISBN: 978-3-662-03448-4
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