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The Formation of Resonance Lines in Gaseous Nebulae Partially Filled with Dust

Published online by Cambridge University Press:  18 September 2017

R. Wehrse
R. Wehrse*
Affiliation:
Institut für Theoretische Astrophysik der Universität Heidelberg, Im Neuenheimer Feld 294, D-6900 Heidelberg, FRG

Extract

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The radiation field for a resonance line is calculated for a gaseous nebula which consists of a dust-free and a dust filled layer (1/2 or 1/4 of the total volume). For comparison we compute also the line profiles for corresponding homogeneous configurations, with and without dust.

Type
Abstracts of Contributed Papers
Information
Symposium - International Astronomical Union , Volume 103: Planetary Nebulae , 1983 , pp. 519
Copyright
Copyright © Reidel 1983