2002/10/18 by A. Cavaliere, Andrea Lapi, A. Lapi +1 · 14 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.1086/345890
published as Astrophys.J. 581 (2002) L1 · 4 pages, 2 figures, uses AASTeX and emulateapj5.sty
arxiv created 2002/10/18 · openalex publication_date 2002/12/02 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31
Galaxy groups are quite underluminous in X-rays compared to clusters, so the intracluster medium (ICM) has to be considerably underdense in the former. We consider this to be due to substantial energy fed back into the ICM when the baryons in the member galaxies condense into stars ending up in supernovae (SNe) or accrete onto central supermassive black holes energizing active galactic nuclei (AGNs). We compute the outflow and the blowout effects driven by the AGNs and the resulting steep luminosity-temperature correlation L X - T . We compare this with the SN contribution and with the X-ray data; the latter require the AGN energy to be coupled to the surrounding ICM at fractional levels around 5 × 10 -2 . We link the L X - T behavior with the parallel effects of the AGN feedback on the gas in the host galaxy; we find that these yield a correlation steep up to M BH ∝ σ 5 between the galactic velocity dispersions and the central black hole masses.