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The Boomerang PWN G106.6+2.9 and the Magnetic Field Structure in Pulsar Wind Nebulae
Kothes, Reich, & Uyanıker 2006 The Astrophysical Journal 638 225.
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.
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.