The Kookaburra's Northern Wing: PWN or SNR?

Computer Science

Scientific paper

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Galactic, Atca

Scientific paper

We propose to image the Northern wing of the Kookaburra complex at 20/13 and 6 cm wavelengths in order to determine if the spectrum is consistent with that of a pulsar wind nebula (PWN), a supernova remnant (SNR) shell, or if it is a composite spectrum with the region near PSR J1420-6048 being different than the rest of the wing. This is crucial to understand both the nature of the wing and to interpret the Very High Energy (> 1 TeV) emission from this object.

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