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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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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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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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Solar And Astrophysical Dynamos And Magnetic Activity (Iau S

instabilities. The goal of IAU Symposium 294 was to discuss the most important results of recent studies of the cosmic dynamo processes, from planets to;

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The Intriguing Life of Massive Galaxies (Iau S295)

in the early Universe, through their evolution with cosmic time to massive galaxies in the local Universe. Key contributions deal with recent and;

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Spectral Energy Distribution Of Galaxies - Sed 2011 (Iau S28

components of the interstellar medium, and high-energy processes involving cosmic rays. IAU Symposium 284 details progress in the development of such;

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

galaxies and black holes evolve over cosmic time.;

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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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Cosmic Magnetic Fields (Iau S259)

Cosmic magnetic fields play a key role in the formation, structure and evolution of planets, stars and galaxies, and possibly the Universe;

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Why Galaxies Care about AGB Stars (IAU S343)

cosmic dust. They are prime laboratories for studying situations where different physical and chemical processes work simultaneously, on;

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Uncovering Early Galaxy Evolution in the ALMA and JWST Era (IAU S352)

The first three billion years of cosmic time were the prime epoch of galaxy formation. Characterising galaxies at this epoch is therefore;

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The Cosmic Dynamo

The 157th IAU Symposium The Cosmic Dynamo was entirely dedicated to dynamo processes, which are fundamental to all cosmic scales. Dynamo;

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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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The Zeldovich Universe (Iau S308)

of cosmic structure. IAU Symposium 308 marked the centenary of the birth of the Russian physicist and cosmologist Yakov B. Zeldovich (1914-87), who;

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Cosmic Collisions

cosmic collisions between galaxies. Hubble's images are snapshots in time and catch the colliding galaxies in different stages of collision;

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Mass-Transfer Induced Activity in Galaxies

large-scale properties of the host galaxy. The crucial question is what triggers and fuels nuclear activity now and at earlier epochs? The;

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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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Massive Stars As Cosmic Engines (Iau S250)

explosions which enrich galaxies in elements such as oxygen, and sometimes their demise is associated with intense bursts of gamma-rays. IAU;

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Astroquizzical: Solving the Cosmic Puzzles of Our Planets, Stars, and Galaxies

journey through outer space, traveling back in time from Earth to the stars and galaxies to the cosmic explosions of the Big Bang.

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From Interstellar Clouds to Star-Forming Galaxies (IAU S315)

The link between the structure of the interstellar medium in galaxies and the star formation process is a fast-growing area;

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

overwhelming evidence in favour of the presence of supermassive black holes at the centre of galaxies, including the Milky Way; of stellar-mass black;

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New Horizons In Time Domain Astronomy (Iau S285)

IAU Symposium 285 addresses studies of variability among the whole gamut of cosmic objects. While new fields involving transients, blazars;

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Star Clusters (IAU S351)

Stellar cluster research is in a dynamic state. IAU Symposium 351 (also chosen as MODEST-19, within the 'Modelling and Observing DEnse;

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Multiwavelength Agn Surveys and Studies (Iau S304)

Active galactic nuclei (AGN) are among the most interesting astrophysical objects in the Universe. IAU Symposium 304, dedicated to marking;

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Galaxies at High Redshift

missions, allow astronomers to directly observe galaxy assembly over cosmic time. These developments demand that scientists are trained in the;

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The Vision of Cosmic Universe to Prem Universe-1995

Galaxies, Spherical and Elliptical Galaxies, Cosmic Functions and Cosmic Sources. How to define the Universe? Cosmic Universe beyond PREM (Field;

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Astrophysics with Radioactive Isotopes

chemical evolution of cosmic gas. Reference materials and explanations are included for students in advanced stages of their education. Nuclear;

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