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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. 1.

Sample spectra of windows used to find Zeeman pairs. Squares and triangles mark RCP and LCP emission, respectively. Gaussian fits to the lines are shown, and lines and features are numbered for reference. The number in the upper right corner marks the transition frequency, in MHz. (ad) Windows in G351.775−0.538, G032.744−0.076, K3−50, and G045.465+0.047. The 1665 and 1667 MHz windows in (a) and (c) are centered at approximately the same position. The magnetic field and center velocity deduced from Zeeman splitting are shown in (a).

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