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相关论文: The AGN/Normal Galaxy Connection : Summary

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The existence of correlations between nuclear properties of galaxies, such as the mass of their central black holes, and larger scale features, like the bulge mass and luminosity, represent a fundamental constraint on galaxy evolution.…

宇宙学与河外天体物理 · 物理学 2015-06-11 G. La Mura , D. Bindoni , S. Ciroi , V. Cracco , R. D'Abrusco , P. Rafanelli , L. Vaona

I discuss some recent observational results in the research of nearby active galactic nuclei (AGN). These results cover three main topics: (i) evidences for the current paradigm for AGN's, which include a nuclear supermassive blackhole…

天体物理学 · 物理学 2007-05-23 Thaisa Storchi-Bergmann

In recent years deep X-ray and infrared surveys have provided an efficient way to find accreting supermassive black holes, otherwise known as active galactic nuclei (AGN), in the young universe. Such surveys can, unlike optical surveys,…

天体物理学 · 物理学 2007-12-10 C. Megan Urry , E. Treister

Our understanding of the cosmic evolution of supermassive black holes (SMBHs) has been revolutionized by the advent of large multiwavelength extragalactic surveys, which have enabled detailed statistical studies of the host galaxies and…

星系天体物理 · 物理学 2016-12-16 Ryan C. Hickox , Stephanie M. LaMassa , John D. Silverman , Alexander Kolodzig

Active galactic nuclei (AGN) are supermassive black holes with luminous accretion disks found in some galaxies, and are thought to play an important role in galaxy evolution. However, traditional optical spectroscopy for identifying AGN…

星系天体物理 · 物理学 2022-12-16 Ziting Guo , John F. Wu , Chelsea E. Sharon

Active Galactic Nuclei (AGN) are known to show flux variability over all observable timescales and across the entire electromagnetic spectrum. Over the past decade, a growing number of sources have been observed to show dramatic flux and…

星系天体物理 · 物理学 2022-11-11 Claudio Ricci , Benny Trakhtenbrot

Dual active galactic nuclei (AGNs) and offset AGNs are kpc-scale separation supermassive black holes pairs created during galaxy mergers, where both or one of the black holes are AGNs, respectively. These dual and offset AGNs are valuable…

Active Galactic Nuclei (AGN) are intensely accreting supermassive black holes at the centers of massive galaxies. Though these objects occupy little spatial extent of the galaxy itself, they are thought to have far reaching affects,…

星系天体物理 · 物理学 2023-07-24 Rachel Cionitti , Brandon Coleman , Allison Kirkpatrick , Greg Troiani

Active Galactic Nuclei are fueled from material (gas or stars) that are in general far away from the gravitational influence of the central black hole, the engine thought to be responsible for their activity. The required material has a lot…

天体物理学 · 物理学 2016-11-03 F. Combes

Active Galactic Nuclei (AGN) represent the growth phases of the supermassive black holes in the center of almost every galaxy. Powerful, highly ionized winds, with velocities $\sim 0.1- 0.2c$ are a common feature in X--ray spectra of…

星系天体物理 · 物理学 2015-09-23 Andrew King , Ken Pounds

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

Active Galactic Nuclei (AGN) are powered by the accretion of material onto a supermassive black hole (SMBH), and are among the most luminous objects in the Universe. However, the huge radiative power of most AGN cannot be seen directly, as…

星系天体物理 · 物理学 2018-10-17 Ryan C. Hickox , David M. Alexander

The role of stars and starbursts in AGN has been a recurring issue for nearly as long as AGN have been recognized as hosts of interesting phenomena. The heated ``starburst X monster'' controversy of the 80's and 90's was gradually replaced…

天体物理学 · 物理学 2009-11-10 Roberto Cid Fernandes

There is growing interest in the possible link between the growth of supermassive black holes and the effect of feedback from them on galaxy growth. There are three areas of significant uncertainty: (i) the physics of the feedback; (ii) the…

天体物理学 · 物理学 2007-05-23 L. Miller

Energy feedback, either from active galactic nuclei (AGN) or from supernovae, is required to understand galaxy formation within a $\Lambda$-Cold Dark Matter cosmology. We study a sample of 127 low-mass galaxies, comparing their stellar…

星系天体物理 · 物理学 2018-03-28 Ignacio Martin-Navarro , Mar Mezcua

It is not yet clear what triggers the activity of active galactic nuclei (AGNs), but galaxy merging has been suspected to be one of the main mechanisms fuelling the activity. Using deep optical images taken at various ground-based…

星系天体物理 · 物理学 2015-05-04 Jueun Hong , Myungshin Im , Minjin Kim , Luis C. Ho

This volume presents an overview of selected aspects of physical processes occurring in the inner regions of Active Galactic Nuclei (AGN). The observational evidence suggests that strong gravitational fields play a significant role in…

高能天体物理现象 · 物理学 2021-11-22 Vladimir Karas , Jiri Svoboda , Michal Zajacek

It has long been suspected that Active Galactic Nuclei are powered by accretion of matter onto massive black holes and this belief implies their presence in the nuclei of most nearby galaxies as "relics" of past activity. Just a few years…

天体物理学 · 物理学 2007-05-23 Alessandro Marconi

The relationship of an AGN to its host galaxy is a crucial question in the study of galaxy evolution. We perform stellar population synthesis in the central regions of galaxies of different activity levels. A large number of stellar…

天体物理学 · 物理学 2007-05-23 C. Boisson , M. Joly

Over the last five decades, AGN studies have produced a number of spectacular examples of synergies and multifaceted approaches in astrophysics. The field of AGN research now spans the entire spectral range and covers more than twelve…

天体物理学 · 物理学 2015-06-24 Andrei P. Lobanov , J. Anton Zensus