  Observations using the Australia Telescope Compact Array at a wavelength of 6
cm have uncovered the radio counterpart to the compact X-ray nebula surrounding
the Vela pulsar. Two lobes were found oriented about the spin axis of the
pulsar, starting at the edge of X-ray emission, they extend to three times the
size. The northern lobe has a bright, defined edge and an integrated flux of
0.14 Jy, while the southern lobe of 0.12 Jy is more diffuse.
