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Energy Distribution of Planetary Nebulae (UV to Radio)

Published online by Cambridge University Press:  07 August 2017

C.Y. Zhang
C.Y. Zhang*
Affiliation:
Department of Astronomy The University of Texas at Austin Austin, TX 78712

Abstract

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The past decade has seen significant progress in our understanding of spectral energy distribution of planetary nebulae over the entire wavelength range from UV to radio. In this review we show the detailed breakdown of the energy budget for a planetary nebula as a system of the three components, i.e., the central star, the gaseous nebula and the dust shell. This picture of the energy distribution is further discussed in the context of planetary nebula evolution.

Type
III. Highlights on the Nebulae
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 99 - 108
Copyright
Copyright © Kluwer 1993 

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