This publication reports the discovery of a pulsar wind nebula in the complex Vela Junior region. Gamma-ray emission from this region has traditionally been attributed to the supernova remnant; however, now thanks to new analysis techniques, we were able to detect emission with distinct properties originating from the position of the pulsar. The emission is consistent with a pulsar wind nebula at this position, which is also detected at both X-ray and radio wavelengths. You can also check out the Source of Month for March 2026, where this source was highlighted.

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Journal reference: Astronomy & Astrophysics 708, A6 (2026)