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Some Properties of Dust in Planetary Nebulae

Published online by Cambridge University Press:  22 September 2016

Nino Panagia
Nino Panagia*
Affiliation:
Laboratorio di Radioastronomia, Bologna, Italy and Laboratorio di Astrofisica Spaziale, Frascati, Italy

Extract

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From an analysis of infrared, optical, ultraviolet and radio data of a number of planetary nebulae, it is found that the dust mixed with the ionized gas mainly consists of relatively large, graphite-like grains.

Type
Session VI: Evolution and Morphology of Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 76: Planetary Nebulae , 1978 , pp. 292
Copyright
Copyright © Reidel 1978