Innermost collimation structure of the M87 jet down to ~ten Schwarzschild radii
Kazuhiro Hada, Motoki Kino, Akihiro Doi, Hiroshi Nagai, Mareki Honma,, Yoshiaki Hagiwara, Marcello Giroletti, Gabriele Giovannini, Noriyuki, Kawaguchi

TL;DR
This study uses multi-frequency VLBA data to analyze the innermost structure of the M87 jet down to about ten Schwarzschild radii, revealing a smooth transition in jet collimation profile and possible shape change near the black hole.
Contribution
First detailed measurement of the M87 jet's collimation profile down to ~10 Schwarzschild radii, linking core size and position across multiple frequencies.
Findings
Jet width scales with frequency as W_c(ν) ∝ ν^{-0.71}
Collimation profile connects smoothly to outer parabolic jet structure
Possible change from parabolic to more radial shape near the black hole
Abstract
We investigated the detailed inner jet structure of M87 using the Very Long Baseline Array data at 2, 5, 8.4, 15, 23.8, 43, and 86 GHz, especially focusing on the multi-frequency properties of the radio core at the jet base. First, we measured a size of the core region transverse to the jet axis, defined as , at each frequency \nu, and found a relation between and as . Then, by combining and the frequency dependence of the core position , which was obtained by our previous study, we have constructed a collimation profile of the innermost jet down to ~10 Schwarzschild radii () from the central black hole. We found that smoothly connects with the width profile of the outer edge-brightened, parabolic jet, and then follows a similar radial…
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