Blowing cold flows away: The impact of early AGN activity on the formation of a brightest cluster galaxy progenitor

Yohan Dubois, Christophe Pichon, Julien Devriendt, Joseph Silk, Martin Haehnelt, Taysun Kimm, Adrianne Slyz

Research output: Contribution to journalArticle

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Abstract

Supermassive black holes (BH) are powerful sources of energy that are already in place at very early epochs of the Universe (by z = 6). Using hydrodynamical simulations of the formation of a massive Mvir = 5 × 1011M⊙ halo by z = 6 (the most massive progenitor of a cluster of Mvir =2×1015M⊙ at z=0), we evaluate the impact of active galactic nuclei (AGN) on galaxy mass content, BH self-regulation and gas distribution inside this massive halo. We find that supernova feedback has a marginal influence on the stellar structure, and no influence on the mass distribution on large scales. In contrast, AGN feedback alone is able to significantly alter the stellar-bulge mass content by quenching star formation when the BH is self-regulating, and by depleting the cold gas reservoir in the centre of the galaxy. The growth of the BH proceeds first by a rapid Eddington-limited period fed by direct cold filamentary infall. When the energy delivered by the AGN is sufficiently large to unbind the cold gas of the bulge, the accretion of gas on to the BH is maintained by both smooth gas inflow and clump migration through the galactic disc triggered by merger-induced torques. The feedback from the AGN has also a severe consequence on the baryon mass content within the halo, producing large-scale hot superwinds, able to blow away some of the cold filamentary material from the centre and reduce the baryon fraction by more than 30 per cent within the halo's virial radius. Thus, in the very young universe, AGN feedback is likely to be a key process, shaping the properties of the most massive galaxies.

Original languageEnglish
Pages (from-to)2885-2900
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume428
Issue number4
DOIs
Publication statusPublished - 2013 Feb 19

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blowing
active galactic nuclei
galaxies
halos
gas
cold gas
baryons
universe
gases
stellar structure
torque
automatic control
merger
energy
clumps
inflow
mass distribution
accretion
supernovae
star formation

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Dubois, Yohan ; Pichon, Christophe ; Devriendt, Julien ; Silk, Joseph ; Haehnelt, Martin ; Kimm, Taysun ; Slyz, Adrianne. / Blowing cold flows away : The impact of early AGN activity on the formation of a brightest cluster galaxy progenitor. In: Monthly Notices of the Royal Astronomical Society. 2013 ; Vol. 428, No. 4. pp. 2885-2900.
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Blowing cold flows away : The impact of early AGN activity on the formation of a brightest cluster galaxy progenitor. / Dubois, Yohan; Pichon, Christophe; Devriendt, Julien; Silk, Joseph; Haehnelt, Martin; Kimm, Taysun; Slyz, Adrianne.

In: Monthly Notices of the Royal Astronomical Society, Vol. 428, No. 4, 19.02.2013, p. 2885-2900.

Research output: Contribution to journalArticle

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T2 - The impact of early AGN activity on the formation of a brightest cluster galaxy progenitor

AU - Dubois, Yohan

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AU - Devriendt, Julien

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AU - Slyz, Adrianne

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