Fig. 2 from Interstellar Hydroxyl Masers in the Galaxy. II. Zeeman Pairs and the Galactic Magnetic Field

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

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. 2.

Histogram of the number of Zeeman pairs found with each magnetic field strength, binned by 1 mG. Positive (negative) field strengths represent magnetic fields oriented in the hemisphere away from (toward) the Sun. A best‐fit Gaussian is also shown. The −25.4 mG pair in G081.871+0.781 is excluded for reasons outlined in § 4.3.

Other Images in This Article

Copyright and Terms & Conditions