2001ApJ...561..930C

The distance to the Vela pulsar (PSR B0833-45) has been traditionally assumed to be 500 pc. Although affected by a significant uncertainty, this value stuck to both the pulsar and the supernova remnant. In an effort to obtain a model-free distance measurement, we have applied high-resolution astrometry to the pulsar V∼23.6 optical counterpart. Using a set of five Hubble Space Telescope Wide Field Planetary Camera 2 observations, we have obtained the first optical measurement of the annual parallax of the Vela pulsar. The parallax turns out to be 3.4±0.7 mas, implying a distance of 294^–50₊₇₆ pc, i.e., a value significantly lower than previously believed. This affects the estimate of the pulsar absolute luminosity and of its emission efficiency at various wavelengths and confirms the exceptionally high value of N_e toward the Vela pulsar. Finally, the complete parallax database allows for a better measurement of the Vela pulsar proper motion [µ_αcos(δ)=-37.2±1.2 mas yr^–1; µ_δ=28.2±1.3 mas yr^–1 after correcting for the peculiar motion of the Sun], which, at the parallax distance, implies a transverse velocity of ~65 km.s^–1. Moreover, the proper-motion position angle appears especially well aligned with the axis of symmetry of the X-ray nebula as seen by Chandra. Such an alignment allows us to assess the space velocity of the Vela pulsar to be 81 km.s^–1.