2014/06/01 by Volker Gaibler, V. Gaibler · 7 citations
Physics and Astronomy · #Active galactic nucleus #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Astrophysics and Star Formation Studies #Context (archaeology) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy formation and evolution #Interstellar medium #Physics #Redshift #astro-ph.GA #astro-ph.HE
paper · pdf · doi:10.1002/asna.201412061
published in Astronomische Nachrichten 335(5), 531-536 (Wiley) · 6 pages, 1 figure, published in final form in Reviews in Modern Astronomy, Vol. 26, AN 335, 531. Based on invited talk at annual meeting 2013 of the Astronomische Gesellschaft
openalex publication_date 2014/06/01 · arxiv created 2014/07/08 · arxiv updated 2014/07/10 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Abstract Simulations of feedback by jets from active galactic nuclei (AGN) in the past mostly focused on the interaction at large scales as the circumgalactic medium or intra‐cluster medium for clusters of galaxies. Only in recent years, simulations have included the interaction of jets with a highly inhomogeneous medium as required by a multi‐phase interstellar medium (ISM). At the same time, feedback by AGN has become a common component for cosmological simulations of galaxy evolution to form massive galaxies compatible with observations. I will present some of our recent results and will put them into further context of other feedback simulations and how the opposing effects of positive and negative feedback by jets might be understood in terms of different properties of the ISM. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)