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Infrared Emission Lines in Planetary Nebulae

Published online by Cambridge University Press:  18 September 2017

Harriet L. Dinerstein
Harriet L. Dinerstein*
Affiliation:
NASA Ames Research Center, Moffett Field, California 94035

Abstract

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Advances in infrared spectroscopy have led to the detection of many forbidden fine-structure emission lines in planetary nebulae. Measurements of these lines offer sensitive probes of the physical conditions and ionization structure, and lead to improved abundance determinations. This paper reviews recent observations and discusses the ways in which infrared line measurements can contribute to our knowledge of planetary nebulae.

Type
Section I: Observations of Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 103: Planetary Nebulae , 1983 , pp. 79 - 88
Copyright
Copyright © Reidel 1983 

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