The Magnetic Field of the H~II Region NGC 6334A
L. F. Rodriguez, Y. Gomez, D. Tafoya

TL;DR
This study measures a very strong magnetic field in the H II region NGC 6334A using Faraday rotation of an extragalactic radio source, revealing insights into magnetic properties of dense star-forming regions.
Contribution
First measurement of a magnetic field as large as 36 microGauss in an H II region using Faraday rotation, highlighting the magnetic flux conservation in dense environments.
Findings
Magnetic field of approximately 36 microGauss in NGC 6334A.
Largest magnetic field measurement for an H II region via this method.
Magnetic to thermal pressure ratio around 5.
Abstract
We have studied the polarization characteristics and Faraday rotation of the extragalactic radio source J172043554, that appears projected on the north lobe of the galactic H II region NGC 6334A. From observations made with the Very Large Array at 6.0 and 3.6 cm in three different epochs (1994, 1997, and 2006), we estimate a rotation measure of +5100900 rad m for the extragalactic source. This large rotation measure implies a line-of-sight average magnetic field of G, the largest obtained by this method for an H II region. NGC 6334A is significantly denser than other H II regions studied and this larger magnetic field is expected on the grounds of magnetic flux conservation. The ratio of thermal to magnetic pressure is 5, in the range of values determined for more diffuse H II regions.
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