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Distribution of Dust in the Orion Nebula

Published online by Cambridge University Press:  14 August 2015

Lindsey F. Smith
Lindsey F. Smith*
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.

Abstract

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The distribution of the dust is found by comparing 3-cm brightness temperatures, Hα surface brightness, and Hβ surface brightness. The dust is probably mixed with the gas. The Balmer radiation originates in front of the dark bay.

Type
Part 2: Galactic H ii Regions
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 257 - 258
Copyright
Copyright © Reidel 1974 

References

Schraml, J. and Mezger, P. G.: 1969, Astrophys. J. 156, 269.CrossRefGoogle Scholar
Wink, J.: 1973, private communication.Google Scholar