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相关论文: Direct effects of the environment on AGN triggerin…

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There is an ongoing debate concerning the driver of nuclear activity in galaxies, with AGN either being triggered by major or minor galactic mergers or, alternatively, through secular processes like cooling gas accretion and/or formation of…

宇宙学与河外天体物理 · 物理学 2014-03-19 Marios Karouzos , Matt J. Jarvis , David Bonfield

We present a study of the prevalence of optical and radio nuclear activity with respect to the environment and interactions in a sample of SDSS galaxies. We defined a local density parameter and a tidal forces estimator and used a cluster…

宇宙学与河外天体物理 · 物理学 2015-06-12 J. Sabater , P. N. Best , M. Argudo-Fernández

We study how AGN activity changes across environments from galaxy pairs to clusters using $143\, 843$ galaxies with $z<0.2$ from the Sloan Digital Sky Survey (SDSS). Using a refined technique, we apply a continuous measure of AGN activity,…

In a series of papers based on the FIRST and Sloan Digital Sky Surveys (SDSS), we investigate the local population of star-forming galaxies and Active Galactic Nuclei (AGN) in order to clarify the link between these two types of activity,…

宇宙学与河外天体物理 · 物理学 2009-03-25 Pietro M. Reviglio , David J. Helfand

Investigating whether and how galaxy mergers affect black hole growth can be determinant for black hole-galaxy evolution models and, in particular, for understanding how early Universe seed black holes grew to become supermassive. However,…

星系天体物理 · 物理学 2025-07-23 A. Eróstegui , M. Mezcua , M. Siudek , H. Domínguez Sánchez , V. Rodríguez Morales

AGN have been generally considered to be less frequent in denser environments due to the lower number of galaxy-galaxy interactions and/or the removal of their gas-rich reservoirs by the dense intergalactic medium. However, recent…

星系天体物理 · 物理学 2023-07-05 B. Rodríguez Del Pino , S. Arribas , A. L. Chies-Santos , I. Lamperti , M. Perna , J. M. Vílchez

We present the observed fraction of galaxies with an Active Galactic Nucleus (AGN) as a function of environment in the Early Data Release of the Sloan Digital Sky Survey (SDSS). Using 4921 galaxies between 0.05 <= z <= 0.095, and brighter…

天体物理学 · 物理学 2010-04-06 Christopher J. Miller , Robert C. Nichol , Percy Gomez , Andrew Hopkins , Mariangela Bernardi

Motivated by the apparently conflicting results reported in the literature on the effect of environment on nuclear activity, we have carried out a new analysis by comparing the fraction of galaxies hosting active galactic nuclei (AGNs) in…

星系天体物理 · 物理学 2019-04-09 Amirnezam Amiri , Saeed Tavasoli , Gianfranco De Zotti

Using two volume-limited Main galaxy samples of the Sloan Digital Sky Survey Data Release 7 (SDSS DR7), we explore influences of galaxy interactions on AGN activity. It is found that in the faint volume-limited sample, paired galaxies have…

宇宙学与河外天体物理 · 物理学 2015-06-11 Xin-Fa Deng , Guisheng Yu , Peng Jiang

We study the properties of SDSS galaxies with and without AGN detection as a function of the local and global environment measured via the local density, the mass of the galaxy host group (parameterised by the group luminosity) and distance…

宇宙学与河外天体物理 · 物理学 2011-04-07 Nelson Padilla , Diego Garcia Lambas , Roberto Gonzalez

Galaxy-galaxy interactions are predicted to cause gas inflows leading to enhanced nuclear star formation. In this paper we test the further prediction that the gas inflows lead to enhanced accretion onto the central supermassive black hole,…

宇宙学与河外天体物理 · 物理学 2015-05-30 Sara L. Ellison , David R. Patton , J. Trevor Mendel , Jillian M. Scudder

Galaxy mass and environment play a major role in the evolution of galaxies. In the transition from star-forming to quenched galaxies, Active galactic nuclei (AGN) have also a principal action. However, the connections between these three…

星系天体物理 · 物理学 2018-12-12 M. Argudo-Fernández , I. Lacerna , S. Duarte Puertas

We present a study of the prevalence and luminosity of Active Galactic Nuclei (AGN; traced by optical spectra) as a function of both environment and galaxy interactions. For this study we used a sample of more than 250000 galaxies drawn…

星系天体物理 · 物理学 2014-11-20 J. Sabater , P. N. Best , T. M. Heckman

Interactions between galaxies are predicted to cause gas inflows that can potentially trigger nuclear activity. Since the inflowing material can obscure the central regions of interacting galaxies, a potential limitation of previous optical…

Environment is one of the key external drivers of the galaxies, while active galactic nucleus (AGN) is one of the key internal drivers. Both of them play fundamental roles in regulating the formation and evolution of galaxies. We explore…

星系天体物理 · 物理学 2019-07-04 Zhong-yi Man , Ying-jie Peng , Xu Kong , Ke-xin Guo , Cheng-peng Zhang , Jing Dou

Using an extensive sample of nearby galaxies (the Nearby Galaxies Catalog, by Tully), we investigate the environment of the galaxies hosting low-luminosity AGNs (Seyferts and LINERs). We define the local galaxy density, adopting a new…

天体物理学 · 物理学 2009-10-22 Pierluigi Monaco , Giuliano Giuricin , Fabio Mardirossian , Marino Mezzetti

We use a sample of close galaxy pairs selected from the Sloan Digital Sky Survey Data Release 4 (SDSS DR4) to investigate in what environments galaxy mergers occur and how the results of these mergers depend on differences in local galaxy…

宇宙学与河外天体物理 · 物理学 2015-05-18 Sara L. Ellison , David R. Patton , Luc Simard , Alan W. McConnachie , Ivan K. Baldry , J. Trevor Mendel

What triggers AGN in some galaxies and what role does this brief period of activity play in the overall evolution of galaxies are still open questions. This paper explores whether or not the local, on scales of $\approx$1\,Mpc, galaxy…

星系天体物理 · 物理学 2025-10-03 Jason Reeves , Anna Sajina , Henry Adair , Duncan Farrah , Mark Lacy

The Sloan Digital Sky Survey (SDSS) has proved to be a powerful resource for understanding the physical properties and chemical composition of star-forming galaxies in the local universe. The SDSS population of active galactic nuclei (AGN)…

星系天体物理 · 物理学 2020-06-17 Sophia R. Flury , Edward C. Moran
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