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Co-evolution of Central Black Holes and Galaxies (IAU S267)

tracers of the evolution of galaxies; they are agents of that evolution. The central black holes in galaxies grow by accretion during a quasar;

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Nuclear Activity in Galaxies Across Cosmic Time (IAU S356)

galaxies; and AGN evolution. IAU S356 was the third IAU symposium organised in Africa in the past 100 years since the IAU was established, and the;

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Black Holes from the Stars to Galaxies--Across the Range of Masses

holes in binary stellar systems; and, possibly, of intermediate-mass black holes in ultraluminous X-ray sources in nearby galaxies. Black holes;

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Extragalactic Jets from Every Angle IAU

Extragalactic jets provide the direct observational evidence for a connection between supermassive black holes and their surrounding cosmic;

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Star Clusters (IAU S351)

dynamical evolution of stellar clusters, and the production of exotic objects such as black holes within stellar clusters. This volume also includes;

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The Intriguing Life of Massive Galaxies (Iau S295)

The lives of massive galaxies are affected by many key processes, including gas accretion and star formation, feedback and quenching, black;

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Joint Evolution of Black Holes and Galaxies

supermassive black holes and the joint evolution of black holes and galaxies to the cold dark matter paradigm of hierarchical galaxy formation and from;

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Dynamics and Evolution of Galactic Nuclei

: supermassive black holes. Connected to the evolution of the galaxies that contain these black holes, galactic nuclei are the sites of uniquely;

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Dynamics and Evolution of Galactic Nuclei

: supermassive black holes. Connected to the evolution of the galaxies that contain these black holes, galactic nuclei are the sites of uniquely;

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Galaxy Evolution and Feedback across Different Environments (IAU S359)

The goal of IAU Symposium 359 on 'Galaxy Evolution and Feedback across Different Environments' (GALFEED) was to bring together the active;

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Multiwavelength Agn Surveys and Studies (Iau S304)

in galaxies and clusters, their host galaxies and environments, binary AGN and merging supermassive black holes, AGN variability, and future large;

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Galaxy Formation and Evolution

of spiral and elliptical galaxies; central supermassive black holes and the activity associated with them; galaxy interactions; and the;

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Spectral Energy Distribution Of Galaxies - Sed 2011 (Iau S28

nearby galaxies, connecting the latter with models for the evolution of the SEDs of distant galaxies and the extragalactic background light. IAU;

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Mass-Transfer Induced Activity in Galaxies

topics covered here are gas flows near to massive black holes, the circumnuclear galactic regions, and the large-scale bars in disk galaxies;

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Galactic Dynamics in the Era of Large Surveys (IAU S353)

Galactic dynamics is fundamental to understanding the formation of galaxies, their internal evolution and their current structure. While;

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Dwarf Galaxies (IAU S344)

Dwarf galaxies are important tools for understanding structure formation and galaxy evolution across cosmic time. These low-mass systems;

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Secular Evolution Of Galaxies

slow dynamical evolution due to internal processes induced by a galaxy's spiral arms, bars, galactic winds, black holes and dark matter haloes;

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Encyclopedia of Space Science Research

science applications of aerogels; dynamics and disruption mechanisms of asteroids; primordial black holes, formation and evolution; black holes;

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Black Hole Astrophysics 2002, Proceedings Of The Sixth Apctp Winter School

of galactic black holes and new understanding of supermassive black holes in AGNs and normal galaxies are also discussed.;

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Proceedings of the International Astronomical Union Symposia and Colloquia

observations, from stars and stellar orbits through nearby black holes and explosive events, to the building blocks and transport of energy in galaxies;

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Galaxies In 3D Across The Universe IAU S

IAU Symposium 309 contains contributions on the timely theme of spatially and energetically resolved properties of galaxies. New;

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Revealing The Heart Of The Galaxy

luminous objects in the Universe - quasars and radio galaxies - are powered by massive black holes at their hearts. But how did black holes emerge;

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The Physics and Evolution of Active Galactic Nuclei

spectroscopy, star formation, and the cosmological evolution of galaxies and black holes. This new text by Hagai Netzer, a renowned astronomer and;

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Formation and Evolution of Galaxy Outskirts (IAU S321)

, to deepen our knowledge of the assembly and evolution of these elusive regions and to establish their role within the evolution of galaxies;

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Proceedings of the International Astronomical Union Symposia and Colloquia

Black holes lie at the heart of some of the most fascinating astrophysical phenomena. IAU Symposium 324 marked the 100th anniversary;

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Galaxy Masses As Constraints of Formation Models

measure the masses of stars, gas and dark matter in galaxies, and explores what these mass determinations tell us about galaxy evolution. A key;

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Astrophysical Dynamics (IAU S271)

nonlinear states and turbulence play a central role. Understanding the behaviour and evolution of such systems requires high-accuracy, multi-scale;

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