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Radiative Transfer Problems in Planetary Nebulae
Published online by Cambridge University Press: 18 September 2017
Extract
In view of the enormous importance of the UV observations of planetary nebulae made possible by the IUE, this review will concentrate primarily on the formation of resonance lines in nebulae; an important special case is that of He II Lyα and its role in the Bowen mechanism. Special attention is given to the effects of dust on the line and continuum formation.
- Type
- Section II: Physical Processes in Planetary Nebulae
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- Copyright
- Copyright © Reidel 1983
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