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The Radio Continuum Morphology of the Orion Nebula

Published online by Cambridge University Press:  12 April 2016

Marcello Felli ,
Ed Churchwell  and
Douglas O. S. Wood
Marcello Felli
Affiliation:
Osservatorio di Arcetri, Largo E. Fermi 5, 50125, Florence, Italy
Ed Churchwell
Affiliation:
University of Wisconsin, 475 N. Charter St., Madison, WI 53706, U.S.A.
Douglas O. S. Wood
Affiliation:
Center for Astrophysics, 60 Garden St., Cambridge, Mass 02138, U.S.A.

Extract

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The Orion Nebula is the bench mark galactic HII region in which major advances have been made in our understanding of the ionization structure, energy balance, plasma dynamics, star formation and interactions of ionized plasmas with dense molecular clouds. Most of these studies require accurate comparison with radio continuum images.

Type
IV. The Orion Nebula
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 315 - 322
Copyright
Copyright © Springer-Verlag 1989

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