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Observations of magnetic fields toward the star forming region S88B
Published online by Cambridge University Press: 01 November 2008
Abstract
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We present observations of the high mass star forming region S88B taken with the VLA with the aim of measuring magnetic fields via the Zeeman effect. By observing thermal absorption lines of OH at 1665 and 1667 MHz, we obtain magnetic fields between 90 and 210 μG. We find these magnetic fields to be dynamically significant in this region.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S259: Cosmic Magnetic Fields: From Planets, to Stars and Galaxies , November 2008 , pp. 99 - 100
- Copyright
- Copyright © International Astronomical Union 2009
References
Roberts, D. A., Crutcher, R. M., Troland, T. H., & Goss, W. M. 1993, ApJ 412, 675CrossRefGoogle Scholar
Sarma, A. P., Troland, T. H., Roberts, D. A., & Crutcher, R. M. 2000, ApJ 533, 271CrossRefGoogle Scholar
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