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Observations of Linear Polarization at 32 Ghz of the Galactic Center Arc

Published online by Cambridge University Press:  23 September 2016

Wolfgang Reich
Wolfgang Reich*
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-5300 Bonn 1, FRG

Abstract

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The Galactic Center Arc has been observed with the Effelsberg 100-m telescope at 32 GHz. The percentage polarization is of the order of 50%. The magnetic field structure is uniform in a direction parallel to the Arc.

Type
The Arc
Information
Symposium - International Astronomical Union , Volume 136: The Galactic Center , 1989 , pp. 265 - 267
Copyright
Copyright © Kluwer 1989 

References

Morsi, H.W., Reich, W.: 1986, Astron. Astrophys. 163, 313 Google Scholar
Reich, W., Sofue, Y., Wielebinski, R., Seiradakis, J.H.: 1988, Astron. Astrophys. 191, 303 Google Scholar
Sofue, Y., Reich, W., Inoue, M., Seiradakis, J.H.: 1987, Publ. Astron. Soc. Japan 39, 95 Google Scholar
Yusef-Zadeh, F., Morris, M., Chance, D.: 1984, Nature 310, 557 Google Scholar
Yusef-Zadeh, F., Morris, M.: 1987, Astrophys. J. 322, 721 CrossRefGoogle Scholar