{ "id": "2006.12519", "version": "v1", "published": "2020-06-22T18:00:05.000Z", "updated": "2020-06-22T18:00:05.000Z", "title": "Physical Conditions and Particle Acceleration in the Kiloparsec Jet of Centaurus A", "authors": [ "Takahiro Sudoh", "Dmitry Khangulyan", "Yoshiyuki Inoue" ], "comment": "Main text 6 pages, 2 figures. Comments welcome", "categories": [ "astro-ph.HE", "astro-ph.GA" ], "abstract": "The non-thermal emission from the kiloparsec-scale jet of Centaurus A exhibits two notable features, bright diffuse emission and many compact knots, which have been intensively studied in X-ray and radio observations. H.E.S.S. recently reported that the very-high-energy gamma-ray emission from this object is extended along the jet direction beyond a kiloparsec from the core. Here, we combine these observations to constrain the physical conditions of the kpc-jet and study the origin of the non-thermal emission. We show that the diffuse jet is weakly magnetized ($\\eta_B\\sim10^{-2}$) and energetically dominated by thermal particles. We also show that knots are the sites of both amplified magnetic field and particle (re-)acceleration. To keep sufficient energy in thermal particles, the magnetic and non-thermal particle energy in the knot regions are tightly constrained. The most plausible condition is an energy equipartition between them, $\\eta_B\\sim\\eta_e\\sim0.1$. Such weak magnetic energy implies that particles in the knots are in the slow cooling regime. We suggest that the entire kpc-scale diffuse emission could be powered by particles that are accelerated at and escaped from knots.", "revisions": [ { "version": "v1", "updated": "2020-06-22T18:00:05.000Z" } ], "analyses": { "keywords": [ "physical conditions", "particle acceleration", "kiloparsec jet", "weak magnetic energy implies", "entire kpc-scale diffuse emission" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }