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相关论文: A Study of High-redshift AGN Feedback in SZ Cluste…

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Feedback from low-excitation radio galaxies (LERGs) plays a key role in the lifecycle of massive galaxies in the local Universe; their evolution, and the impact of these active galactic nuclei on early galaxy evolution, however, remain…

Recent measurements of the abundance of AGN with low-luminosities (L_X< 10^44 erg/s in the 2-10 keV energy band) at high redshifts z>4 provide a serious challenge for Cold Dark Matter (CDM) models based on interaction-driven fueling of AGN.…

宇宙学与河外天体物理 · 物理学 2015-06-15 N. Menci , F. Fiore , A. Lamastra

Several lines of argument support the existence of a link between activity at the nuclei of galaxies, in the form of an accreting supermassive black hole, and star-formation activity in these galaxies. The exact nature of this link is still…

We study the impact of outflows driven by active galactic nuclei (AGN) on galaxy formation. Outflows move into the surrounding intergalactic medium (IGM) and heat it sufficiently to prevent it from condensing onto galaxies. In the dense,…

天体物理学 · 物理学 2009-11-13 Evan Scannapieco , Joseph Silk , Rychard Bouwens

Radio outflows of active galactic nuclei (AGN) are invoked in cosmological models as a key feedback mechanism in the latest phases of massive galaxy formation. Recently it has been suggested that the two major radio AGN populations -- the…

宇宙学与河外天体物理 · 物理学 2011-02-11 V. Smolcic

An understanding of the relationship between radio-loud active galaxies and their large-scale environments is essential for realistic modelling of radio-galaxy evolution and environmental impact, for understanding AGN triggering and life…

X-ray surveys facilitate investigations of the environment of AGNs. Deep Chandra observations revealed that the AGNs source surface density rises near clusters of galaxies. The natural extension of these works is the measurement of spatial…

天体物理学 · 物理学 2009-11-11 N. Cappelluti , H. Boehringer , P. Schuecker , E. Pierpaoli , C. R. Mullis , I. M. Gioia , J. P. Henry

We present new, deep, narrow- and broad-band Hubble Space Telescope observations of seven of the most star-forming brightest cluster galaxies (BCGs). Continuum-subtracted [O II] maps reveal the detailed, complex structure of warm ($T \sim…

In a previous paper we showed that the radio sources selected by combining large areas radio and optical surveys, present a strong deficit of radio emission with respect to 3CR radio-galaxies matched in line emission luminosity. We argued…

宇宙学与河外天体物理 · 物理学 2015-05-19 Ranieri D. Baldi , Alessandro Capetti

We compute the cross-correlation between a sample of 14,000 radio-loud AGN (RLAGN) with redshifts between 0.4 and 0.8 selected from the Sloan Digital Sky Survey and a reference sample of 1.2 million luminous red galaxies in the same…

宇宙学与河外天体物理 · 物理学 2011-03-28 Emilio Donoso , Cheng Li , Guinevere Kauffmann , Philip N. Best , Timothy M. Heckman

Low luminosity radio-loud active galactic nuclei (AGN) are generally found in massive red elliptical galaxies, where they are thought to be powered through gas accretion from their surrounding hot halos in a radiatively inefficient manner.…

宇宙学与河外天体物理 · 物理学 2012-06-05 R. M. J. Janssen , H. J. A. Rottgering , P. N. Best , J. Brinchmann

We present an analysis of the 2-10 keV X-ray emission associated with the active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs). Our sample consists of 32 BCGs that lie in highly X-ray luminous cluster of galaxies (L_X-ray…

宇宙学与河外天体物理 · 物理学 2015-06-12 J. Hlavacek-Larrondo , A. C. Fabian , A. C. Edge , H. Ebeling , S. W. Allen , J. S. Sanders , G. B. Taylor

Spatially resolved observations of AGN host galaxies undergoing feedback processes are one of the most relevant avenues through which galactic evolution can be studied, given the long lasting effects AGN feedback has on gas reservoirs, star…

Galaxy cluster abundance provides a powerful probe of the $\Lambda$CDM model and enables precise constraints on cosmological parameters. Millimeter-wavelength surveys detect clusters through the Sunyaev-Zeldovich (SZ) effect, and are…

宇宙学与河外天体物理 · 物理学 2026-05-18 Harshda Saxena , Adam B. Mantz , Jack Sayers , Denise G. Yudovich , Steve W. Allen

An extremely deep 5 GHz radio observation is presented of the rich cluster MS1054-03 at redshift z=0.83. 34 radio sources are detected down to a 32 micro-Jy (6 sigma), compared to about 25 expected from previous blank field radio source…

天体物理学 · 物理学 2009-11-07 P. N. Best , P. G. van Dokkum , M. Franx , H. J. A. Rottgering

We investigate extremely luminous dusty galaxies in the environments around WISE-selected hot dust obscured galaxies (Hot DOGs) and WISE/radio-selected active galactic nuclei (AGNs) at average redshifts of z = 2.7 and z = 1.7, respectively.…

Galaxy clusters at high redshift present a superb opportunity to study galaxy evolution, with large galaxy samples at fixed distances. Several lines of evidence point towards large formation redshifts and passive evolution for cluster…

天体物理学 · 物理学 2009-03-02 S. C. Chapman , P. McCarthy , S. E. Persson

In this study we investigate 89 radio galaxies that are spectroscopically-confirmed to be members of five large scale structures in the redshift range of $0.65 \le z \le 0.96$. Based on a two-stage classification scheme, the radio galaxies…

We explore the processes that trigger local AGN and the role of these AGN in regulating star formation, using ~350 nearby galaxies observed by the mJy Imaging VLBA Exploration at 20cm (mJIVE) survey. The >10^7 K brightness temperature…

星系天体物理 · 物理学 2015-07-15 Sugata Kaviraj , Stanislav S. Shabala , Adam T. Deller , Enno Middelberg
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