2008/08/02 by Suchetana Chatterjee, Tiziana Di Matteo, Arthur Kosowsky +1 · 2 citations
Physics and Astronomy · #Accretion (finance) #Active galactic nucleus #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Black hole (networking) #Cosmic microwave background #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy formation and evolution #Intergalactic travel #Physics #Quasar #Radio Astronomy Observations and Technology #Redshift #Star formation #Sunyaev–Zel'dovich effect #Supermassive black hole #astro-ph
paper · pdf · doi:10.1111/j.1365-2966.2008.13784.x
11 pages, 6 figures, 3 tables (Accepted for publication in MNRAS on July 30th 2008)
arxiv created 2008/08/02 · openalex publication_date 2008/09/10 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Quasar feedback has most likely a substantial but only partially understood impact on the formation of structure in the universe. A potential direct probe of this feedback mechanism is the Sunyaev-Zel'dovich (SZ) effect: energy emitted from quasar heats the surrounding intergalactic medium and induces a distortion in the microwave background radiation passing through the region. Here, we examine the formation of such hot quasar bubbles using a cosmological hydrodynamic simulation which includes a self-consistent treatment of black hole growth and associated feedback, along with radiative gas cooling and star formation. From this simulation, we construct microwave maps of the resulting SZ effect around black holes with a range of masses and redshifts. The size of the temperature distortion scales approximately with black hole mass and accretion rate, with a typical amplitude up to a few micro-Kelvin on angular scales around 10 arcsec. We discuss prospects for the direct detection of this signal with current and future single-dish and interferometric observations, including Atacama Large Millimetre Array (ALMA) and Cornell Caltech Atacama Telescope (CCAT). These measurements will be challenging, but will allow us to characterize the evolution and growth of supermassive black holes and the role of their energy feedback on galaxy formation.