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Are most of the VHE gamma-ray unidentified sources relic PWNe? · Around

2013

Are most of the VHE gamma-ray unidentified sources relic PWNe?

Tibolla, Omar, Vorster, Michael, Kaufmann, Sarah et al.

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The evolution of Pulsar Wind Nebulae (PWNe) plays a crucial role in interpreting the very high energy (VHE; > 10^11 eV) gamma-ray unidentified sources; and moreover it represents the only viable option to explain the discovery of several "dark sources" in the TeV gamma-ray (i.e.

VHE gamma-ray sources without lower energies, radio or X-ray counterparts).
The newest time-dependent modeling of PWNe presented in [1] and [2] has to be tested on a broader sample of young well-known PWNe and applied to the full-sample of "dark sources".
The consequences of this interpretation go far beyond the interpretation of "dark sources": e.g.

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