Evidence of strong quasar feedback in the early Universe - Wikidata - awgldk - TriplyDB

Evidence of strong quasar feedback in the early Universe

Evidence of strong quasar feedback in the early Universe

http://www.wikidata.org/entity/Q58922153

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Strangulation as the primary mechanism for shutting down star formation in galaxies.Stellar feedback as the origin of an extended molecular outflow in a starburst galaxy.Exceptional AGN-driven turbulence inhibits star formation in the 3C 326N radio galaxy Dark-ages reionization and galaxy formation simulation – XIII. AGN quenching of high-redshift star formation in ZF-COSMOS-20115 Properties of the molecular gas in the fast outflow in the Seyfert galaxy IC 5063 High-resolution imaging of the molecular outflows in two mergers: IRAS 17208-0014 and NGC 1614 Models of AGN feedback Molecular line emission in NGC 1068 imaged with ALMA Fueling the central engine of radio galaxies. III. Molecular gas and star formation efficiency of 3C 293 Blowing cold flows away: the impact of early AGN activity on the formation of a brightest cluster galaxy progenitor The origin of the far-infrared continuum of z ~ 6 quasars. A radiative transfer model for SDSS J1148+5251 On the Formation of the First Quasars Planck’s Dusty GEMS The assembly of ‘normal’ galaxies atz ∼ 7 probed by ALMA The XMM deep survey in the CDF-S A fast ionised wind in a star-forming quasar system atz~ 1.5 resolved through adaptive optics assisted near-infrared data Galaxy-wide outflows inz~ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopy X-shooter reveals powerful outflows in z ∼ 1.5 X-ray selected obscured quasi-stellar objects ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole at z = 4.75 The space density of Compton-thick AGN atz≈ 0.8 in the zCOSMOS-Bright Survey Gas reservoir of a hyper-luminous quasar atz= 2.6 Ionised outflows inz~ 2.4 quasar host galaxies Constraining the nature of two Ly emitters detected by ALMA at z = 4.7 High-resolution C+imaging of HDF850.1 reveals a merging galaxy atz= 5.185 Tracing outflows in the AGN forbidden region with SINFONI AGN wind scaling relations and the co-evolution of black holes and galaxies The multi-phase winds of Markarian 231: from the hot, nuclear, ultra-fast wind to the galaxy-scale, molecular outflow Very extended cold gas, star formation and outflows in the halo of a bright quasar atz> 6 The WISSH quasars project

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Evidence of strong quasar feedback in the early Universe

http://www.wikidata.org/entity/Q58922153

description

article

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована в липні 2012

@uk

name

Evidence of strong quasar feedback in the early Universe

@en

Evidence of strong quasar feedback in the early Universe

@nl

type

label

Evidence of strong quasar feedback in the early Universe

@en

Evidence of strong quasar feedback in the early Universe

@nl

prefLabel

Evidence of strong quasar feedback in the early Universe

@en

Evidence of strong quasar feedback in the early Universe

@nl

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J.1745-3933.2012.01303.X

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Monthly Notices of the Royal Astronomical Society: Letters

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Evidence of strong quasar feedback in the early Universe

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A. Ferrara

http://www.w3.org/2001/XMLSchema#string

E. Piconcelli

http://www.w3.org/2001/XMLSchema#string

E. Sturm

http://www.w3.org/2001/XMLSchema#string

L. J. Tacconi

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R. Neri

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S. Gallerani

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P2860

Molecular gas in the host galaxy of a quasar at redshift z = 6.42.

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

The suppression of star formation by powerful active galactic nuclei

High-excitation CO in a quasar host galaxy atz $\mathsf{=6.42}$

350 μm Dust Emission from High‐Redshift Quasars

Discovery of an active galactic nucleus driven molecular outflow in the local early-type galaxy NGC 1266

Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation

Searching for evidence of energetic feedback in distant galaxies: a galaxy wide outflow in az ≈ 2ultraluminous infrared galaxy

Direct evidence for termination of obscured star formation by radiatively driven outflows in reddened QSOs

The density of very massive evolved galaxies to z = 1.7

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L66-L70

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scholarly article

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10.1111/J.1745-3933.2012.01303.X

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1

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425

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Roberto Maiolino

Chiara Feruglio

Reinhard Genzel

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2012-07-09T00:00:00Z

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1204.2904

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2012MNRAS.425L..66M

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