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SiO Emission from the Orion Nebula

Published online by Cambridge University Press:  14 August 2015

B. Baud ,
J. H. Bieging ,
R. L. Plambeck ,
D. D. Thornton ,
W. J. Welch  and
M.C.H. Wright
B. Baud
Affiliation:
Radio Astronomy Lab, University of California, Berkeley
J. H. Bieging
Affiliation:
Radio Astronomy Lab, University of California, Berkeley
R. L. Plambeck
Affiliation:
Radio Astronomy Lab, University of California, Berkeley
D. D. Thornton
Affiliation:
Radio Astronomy Lab, University of California, Berkeley
W. J. Welch
Affiliation:
Radio Astronomy Lab, University of California, Berkeley
M.C.H. Wright
Affiliation:
Radio Astronomy Lab, University of California, Berkeley

Abstract

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SiO emission in both a strong maser transition in the first excited vibrational state and in a weaker transition in the ground vibrational state both arise from the same small region in the Kleinmann-Low Nebula in Orion. Within the errors, the source position coincides with that of the infrared source IRc2.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 545 - 548
Copyright
Copyright © Reidel 1980 

References

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