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Further Observational Studies of the High Velocity Molecular Source (“Plateau”) in Orion

Published online by Cambridge University Press:  14 August 2015

T.B.H. Kuiper ,
E.N. Rodriguez Kuiper  and
B. Zuckerman
T.B.H. Kuiper
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology
E.N. Rodriguez Kuiper
Affiliation:
Western Laboratories, Ball Aerospace Systems Divisions
B. Zuckerman
Affiliation:
Astronomy Program, University of Maryland

Abstract

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Sensitive measurements have been made of the profiles of various molecular lines in the direction of the BN/KL infrared complex in Orion. Similar line shapes are found for the high velocity wings (“plateau”) of most lines observed. The position of the high velocity source (HVS) was found in SO and HCO+ relative to the SiO maser. A search for HV emission in other sources was unsuccessful.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 31 - 32
Copyright
Copyright © Reidel 1980 

References

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