2006/06/07 by M. Perucho, A. P. Lobanov, A. Lobanov +4 · 69 citations
Physics and Astronomy · #Active galactic nucleus #Astrophysical Phenomena and Observations #Astrophysical jet #Astrophysics #Astrophysics and Cosmic Phenomena #Classical mechanics #Context (archaeology) #Galaxy #Gamma-ray bursts and supernovae #Geology #Helmholtz free energy #Instability #Jet (fluid) #Mechanics #Physics #Quantum mechanics #Relativistic beaming #astro-ph
paper · pdf · doi:10.1051/0004-6361:20065310
published in Astronomy and Astrophysics 456(2), 493-504 (EDP Sciences) · Accepted for publication in Astronomy & Astrophysics. 14 pages. Higher resolution plots available on request to [email protected] and at http://www.mpifr-bonn.mpg.de/staff/mperucho
arxiv created 2006/06/07 · openalex publication_date 2006/08/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Context.Relativistic outflows represent one of the best-suited tools to probe the physics of AGN. Numerical modelling of internal structure of the relativistic outflows on parsec scales provides important clues about the conditions and dynamics of the material in the immediate vicinity of the central black holes in AGN.