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Title: Relationship between star formation rate and black hole accretion at z=3: the different contributions in quiescent, normal, and starburst galaxies

We investigate the co-evolution of the black hole accretion rate (BHAR) and the star formation rate (SFR) in 1.5
Authors:
; ;  [1] ; ; ; ;  [2] ; ;  [3] ; ;  [4] ;  [5] ;  [6] ;  [7] ;  [8]
  1. Dipartimento di Fisica e Astronomia “G. Galilei”, Universita’ di Padova, Vicolo dell’Osservatorio 3, I-35122 (Italy)
  2. Dipartimento di Fisica e Astronomia, Università di Bologna, viale Berti Pichat 6/2, I-40127 Bologna (Italy)
  3. Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, IRFU/Service d’Astrophysique, Bât.709, CEA-Saclay, F-91191 Gif-sur-Yvette Cedex (France)
  4. INAF-Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 2, I-35122 Padova (Italy)
  5. Department of Physics and Astronomy, University of Sheffield, S3 7RH (United Kingdom)
  6. Max Planck Institut für Extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching bei München (Germany)
  7. INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127, Bologna (Italy)
  8. Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, The University of Tokyo, Kashiwanoha, Kashiwa 277-8583 (Japan)
Publication Date:
OSTI Identifier:
22364185
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal Letters; Journal Volume: 800; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; BLACK HOLES; COMPARATIVE EVALUATIONS; COMPUTERIZED SIMULATION; CORRELATIONS; FAR INFRARED RADIATION; GALAXIES; GALAXY NUCLEI; LUMINOSITY; MASS; PHOTOMETRY; STAR ACCRETION; STARS; UNIVERSE; X RADIATION