# Pilot KaVA monitoring on the M87 jet: confirming the inner jet structure and superluminal motions at sub-pc scales

## TL;DR

This study used the KaVA array to monitor the M87 jet at 22 GHz, revealing detailed inner jet structure, superluminal motions, and acceleration, confirming these features are fundamental to the jet’s behavior.

## Contribution

First high-cadence KaVA monitoring of M87 jet at 22 GHz, demonstrating its capability to observe superluminal motions and acceleration at sub-parsec scales.

## Key findings

- Detected superluminal motions at 0.1-2 pc scales.
- Observed gradual acceleration of jet components.
- Confirmed similar kinematic features across different instruments.

## Abstract

We report the initial results of our high-cadence monitoring program on the radio jet in the active galaxy M87, obtained by the KVN and VERA Array (KaVA) at 22 GHz. This is a pilot study that preceded a larger KaVA-M87 monitoring program, which is currently ongoing. The pilot monitoring was mostly performed every two to three weeks from December 2013 to June 2014, at a recording rate of 1 Gbps, obtaining the data for a total of 10 epochs. We successfully obtained a sequence of good quality radio maps that revealed the rich structure of this jet from <~1 mas to 20 mas, corresponding to physical scales (projected) of ~0.1-2 pc (or ~140-2800 Schwarzschild radii). We detected superluminal motions at these scales, together with a trend of gradual acceleration. The first evidence for such fast motions and acceleration near the jet base were obtained from recent VLBA studies at 43 GHz, and the fact that very similar kinematics are seen at a different frequency and time with a different instrument suggests these properties are fundamental characteristics of this jet. This pilot program demonstrates that KaVA is a powerful VLBI array for studying the detailed structural evolution of the M87 jet and also other relativistic jets.