Multiwavelength morphology of Vela X. The individual panels show the morphology of nonthermal emission in a 5° × 5° region around the Vela pulsar in a low-frequency radio band (top left), in the nonthermal X-ray regime (top right), and at TeV energies (bottom left). The bottom right panel displays a false-color superposition of the three bands. In the radio and X-ray images, a 3′ radius around the pulsar was masked, before they were smoothed with a Gaussian kernel of σ = 6′ to approximately match the resolution of the TeV band. In all three bands, we used a square-root brightness scale, spanning a factor of 30 in dynamic range.