SIMBAD references

2011ApJ...736...83H - Astrophys. J., 736, 83 (2011/August-1)

Magnetic fields in large-diameter H II regions revealed by the Faraday rotation of compact extragalactic radio sources.

HARVEY-SMITH L., MADSEN G.J. and GAENSLER B.M.

Abstract (from CDS):

We present a study of the line-of-sight magnetic fields in five large-diameter Galactic H II regions. Using the Faraday rotation of background polarized radio sources, as well as dust-corrected Hα surface brightness as a probe of electron density, we estimated the strength and orientation of the magnetic field along 93 individual sight lines through the H II regions. Each of the H II regions displayed a coherent magnetic field. The magnetic field strength (line-of-sight component) in the regions ranges from 2 to 6 µG, which is similar to the typical magnetic field strength in the diffuse interstellar medium. We investigated the relationship between magnetic field strength and electron density in the five H II regions. The slope of magnetic field versus density in the low-density regime (0.8/cm3 < ne<30/cm3) is very slightly above zero. We also calculated the ratio of thermal to magnetic pressure, βth, for each data point, which fell in the range 1.01 < βth< 25. Finally, we studied the orientation of the magnetic field in the solar neighborhood (d < 1.1 kpc) using our data from five H II regions along with existing measurements of the line-of-sight magnetic field strength from polarized pulsars whose distances have been determined from their annual parallax. We identify a net direction for the magnetic field in the solar neighborhood, but find no evidence for a preferred vertical direction of the magnetic field above or below the Galactic plane.

Abstract Copyright:

Journal keyword(s): H II regions - ISM: magnetic fields - polarization - radio continuum: ISM

Simbad objects: 19

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2019.09.21-09:42:42

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