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Polarized Emission in the Broad SiO Feature from R Leo

Published online by Cambridge University Press:  14 August 2015

F. O. Clark ,
D. R. Johnson ,
T. H. Troland  and
C. E. Heiles
F. O. Clark
Affiliation:
University of Kentucky
D. R. Johnson
Affiliation:
National Bureau of Standards
T. H. Troland
Affiliation:
University of California at Berkeley
C. E. Heiles
Affiliation:
University of California at Berkeley

Abstract

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Linearly polarized SiO emission spread over 12 km/s has been detected from the star R Leo. The position angle of polarized emission varies systematically with respect to the spectral line center. Interpreted in terms of radiative transfer theory, this change in position angle may be due to magnetorotation, which allows the determination of the magnetic field (9×10−3/cos θ Gauss), and the SiO systemic velocity (−1 ± 2 km/s).

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 543 - 544
Copyright
Copyright © Reidel 1980 

References

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