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Structure in the gas and magnetic field in S106

Published online by Cambridge University Press:  03 August 2017

Richard M. Crutcher
Richard M. Crutcher*
Affiliation:
Astronomy Department, University of Illinois, Urbana, IL 61801, U.S.A.

Abstract

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BIMA molecular-line observations show evidence for an expanding molecular ring around IRS 4, a newly formed massive star at the center of the bipolar nebula S106. VLA observations of the Zeeman effect in the OH 1665 MHz line show that the magnetic field strength is about 1 mG and that it reverses direction from one lobe of the bipolar nebula to the other.

Type
Velocity Field and Magnetic Field
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 61 - 64
Copyright
Copyright © Kluwer 1991