HST-1 as a Window to the Energetics of the Jet Spine of M87
Brian Punsly

TL;DR
This paper interprets the optical knot HST-1 in M87's jet as part of the relativistic spine, providing estimates of the jet's power and insights into the central engine's activity over the past few hundred years.
Contribution
It offers a new interpretation of HST-1 as the jet spine and constrains the historical jet power and efficiency of M87's central engine based on multi-frequency imaging data.
Findings
HST-1 is associated with the relativistic jet spine.
Estimated jet power in the recent past is up to 2 x 10^{42} ergs/s.
The jet production efficiency is approximately 3.5%.
Abstract
A new interpretation of the optical knot in the jet of M87, HST-1, is presented. High sensitivity 22 GHz Very Large Array images locate HST-1 to within 6 mas of the jet axis immediately upstream. 1.7 GHz Very Long Baseline Array images of a bright flare in 2005 indicates that the preponderance of emission in the early stages originates in an elongated region that is tilted from the jet axis. The superluminal motion, shape, location and the large jet-aligned optical/UV polarization suggest an identification with the putative relativistic spine of the jet. As such, energy flux estimates for HST-1, mas from the nucleus, published in 2006 indicate that the central engine injected into the base of the spine years earler. Furthermore, previous studies reveal a tubular protonic jet on sub-mas scales that…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Solar and Space Plasma Dynamics
