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Interstellar Hydroxyl Masers in the Galaxy. II. Zeeman Pairs and the Galactic Magnetic Field

  • Authors: Vincent L. Fish, Mark J. Reid, Alice L. Argon, and Karl M. Menten

Fish et al. 2003 The Astrophysical Journal 596 328.

  • Provider: AAS Journals

Caption: Fig. 4.

Plot of simulated rotation measures generated from magnetic field directions deduced from OH Zeeman splitting. No simulated rotation measures are plotted for Galactic longitudes unsampled by the data of Figs. 3 and 4. The dots represent extragalactic rotation measure data as taken from Rand & Kulkarni (1989) at Galactic latitude ﹩b=-15﹩°, 0°, and 15°. See § 5.3 for further details.

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