MOJAVE XII: Acceleration and Collimation of Blazar Jets on Parsec Scales

TL;DR

This study analyzes the acceleration and collimation of blazar jets on parsec scales, revealing that jet features generally accelerate near the base and then decelerate or stabilize further out, with evidence of jet collimation.

Contribution

It provides the first comprehensive analysis of acceleration and collimation in a large sample of blazar jets, highlighting the dominance of Lorentz factor changes over jet bending.

Findings

Features accelerate within ~10-20 parsecs from the jet base.

Jet features show a broad range of apparent speeds at fixed distances.

Evidence of jet collimation and alignment within ~10 parsecs.

Abstract

We report on the acceleration properties of 329 features in 95 blazar jets from the MOJAVE VLBA program. Nearly half the features and three-quarters of the jets show significant changes in speed and/or direction. In general, apparent speed changes are distinctly larger than changes in direction, indicating that changes in the Lorentz factors of jet features dominate the observed speed changes rather than bends along the line of sight. Observed accelerations tend to increase the speed of features near the jet base, $\lesssim 10-20$ parsecs projected, and decrease their speed at longer distances. The range of apparent speeds at fixed distance in an individual jet can span a factor of a few, indicating that shock properties and geometry may influence the apparent motions; however, we suggest that the broad trend of jet features increasing their speed near the origin is due to an overall acceleration of the jet flow out to de-projected distances of order $10^2$ parsecs, beyond which the flow begins to decelerate or remains nearly constant in speed. We estimate intrinsic rates of change of the Lorentz factors in the galaxy frame of order $\dot{\Gamma}/\Gamma \simeq 10^{-3}$ to $10^{-2}$ per year which can lead to total Lorentz factor changes of a factor of a few on the length scales observed here. Finally, we also find evidence for jet collimation at projected distances of $\lesssim 10$ parsecs in the form of the non-radial motion and bending accelerations that tend to better align features with the inner jet.