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The Boomerang PWN G106.6+2.9 and the Magnetic Field Structure in Pulsar Wind Nebulae

  • Authors: Roland Kothes, Wolfgang Reich, and Bülent Uyanıker

Kothes, Reich, & Uyanıker 2006 The Astrophysical Journal 638 225.

  • Provider: AAS Journals

Caption: Fig. 5.

Sample rotation measure fits of the Boomerang. Data at 1420 MHz, 4.85 GHz, 8.35 GHz, and 10.45 GHz were taken at 2﹩\farcm﹩45 resolution. The top two panels show locations on the Boomerang. The area around the three higher frequencies is magnified to demonstrate the accuracy of the fit. The fits for the "tongue" region are displayed in the two bottom panels. A more detailed description is given in the text (§ 3.3).

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