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Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit - Nature

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Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit - Nature

Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar wind nebula is powered by a young pulsar (B0833-45, aged 11,000 years)1 and located inside an extended structure called Vela X, which is itself inside the supernova remnant2. Previous X-ray observations revealed two prominent arcs that are bisected by a jet and counter jet3,4.

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Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit - Nature

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Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit - Nature

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