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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. 3.

Radio spectrum of the "Boomerang" PWN. The break occurs between 4 GHz and 5 GHz. The spectral indices below and above the break are indicated.

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