The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end - Wikidata - awgldk - TriplyDB

The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end

The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end

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Black-hole-regulated star formation in massive galaxies.Comparing galaxy formation in semi-analytic models and hydrodynamical simulations The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations Cosmic evolution of stellar quenching by AGN feedback: clues from the Horizon-AGN simulation Galaxy metallicity scaling relations in the EAGLE simulations The relation between galaxy morphology and colour in the EAGLE simulation The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies The Hydrangea simulations: galaxy formation in and around massive clusters The link between galaxy and black hole growth in the eagle simulation HSTHα grism spectroscopy of ROLES: a flatter low-mass slope for thez ∼ 1 SSFR–mass relation

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The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end

http://www.wikidata.org/entity/Q56907487

description

article

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im Oktober 2016 veröffentlichter wissenschaftlicher Artikel

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wetenschappelijk artikel

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наукова стаття, опублікована в жовтні 2016

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The dark nemesis of galaxy for ...... bring star formation to an end

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The dark nemesis of galaxy for ...... bring star formation to an end

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The dark nemesis of galaxy for ...... bring star formation to an end

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The dark nemesis of galaxy for ...... bring star formation to an end

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The dark nemesis of galaxy for ...... bring star formation to an end

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The dark nemesis of galaxy for ...... bring star formation to an end

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Monthly Notices of the Royal Astronomical Society

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The dark nemesis of galaxy for ...... bring star formation to an end

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Carlos S. Frenk

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Richard G. Bower

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Planck 2013 results. XVI. Cosmological parameters

A luminous quasar at a redshift of z = 7.085.

Direct formation of supermassive black holes via multi-scale gas inflows in galaxy mergers.

Energy input from quasars regulates the growth and activity of black holes and their host galaxies.

Formation of supermassive black holes by direct collapse in pre-galactic haloes

A deep Chandra observation of the Perseus cluster: shocks and ripples

Energetic galaxy-wide outflows in high-redshift ultraluminous infrared galaxies hosting AGN activity

Revisiting the scaling relations of black hole masses and host galaxy properties

Dark matter halo concentrations in theWilkinson Microwave Anisotropy Probeyear 5 cosmology

The physics driving the cosmic star formation history

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32–44

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scholarly article

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10.1093/MNRAS/STW2735

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1

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465

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Matthieu Schaller

Robert A. Crain

Stuart McAlpine

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2016-10-23T00:00:00Z

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1607.07445

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2017MNRAS.465...32B

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