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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 Intriguing Life of Massive Galaxies (Iau S295)

satellite accretion. These proceedings of IAU Symposium 295 discuss recent progress in galaxy formation and evolution, and plan ahead for future;

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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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Massive Stars As Cosmic Engines (Iau S250)

: atmospheres of massive stars; the physics and evolution of massive stars; massive stars in the nearby Universe; hydrodynamics and feedback from;

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

IAU Symposium 267 assesses the diverse observational and theoretical attempts to answer the complex question of how quasars physically;

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Formation and Evolution of Galaxy Outskirts (IAU S321)

proceedings of IAU Symposium 321 summarize our current understanding of the rarefied universe and prepare for the optimal exploitation of upcoming;

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Galaxy Masses As Constraints of Formation Models

instrumentation be optimized for galaxy evolution studies? And, what future observations would be most useful to constrain the models? IAU S311 offers a;

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Setting The Scene For Gaia And Lamost (Iau S298)

for a billion stars, Gaia is set to transform the way we study the composition, formation and evolution of our galaxy. Concurrently the LAMOST;

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Galaxies In 3D Across The Universe IAU S

graduate students working in areas relating to galaxy formation and evolution, star formation, dust and stellar populations.;

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The Lives and Death-Throes of Massive Stars (IAU S329)

harsh test for the current state-of-the-art theoretical calculations of massive star birth, evolution and death. IAU Symposium 329 covers these;

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

that all aspects of galaxy evolution are strongly influenced by the interplay between the dynamics of stars, gas, and dark matter. IAU;

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Proceedings of the International Astronomical Union Symposia and Colloquia

Planetary nebulae, glowing shells of ionized gas, are the spectacular products of the evolution of low- and intermediate-mass stars. For;

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General Assembly Of Galaxy Halos IAU S31

encompassing stellar and galactic astrophysics and galaxy evolution.;

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Extragalactic Jets from Every Angle IAU

environments. They deliver the energy released by an accreting black hole across large distances and impact the formation and evolution of surrounding;

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Low-Metallicity Star Formation (Iau S255)

developments in six key areas, including: Population III and metal-free star formation; metal-enrichment, chemical evolution and feedback; explosive;

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

understanding of galaxy evolution in the young Universe.;

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Multiwavelength Agn Surveys and Studies (Iau S304)

physical connections between the different classes of AGN; the relation of AGN to their host galaxies; and understanding the true fraction;

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

formation modes from solar system scales to galaxy scales. IAU Symposium 315 aims to build a coherent picture of how star formation is fueled on a;

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Solar And Astrophysical Dynamos And Magnetic Activity (Iau S

Global magnetic fields in planets, in the Sun and other stars, in spiral galaxies and galaxy clusters are believed to be generated and;

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Proceedings of the International Astronomical Union Symposia and Colloquia

abilities to probe details of astronomical sources. Molecular maser emission studies address important questions in the formation and evolution;

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Proceedings of the International Astronomical Union Symposia and Colloquia

Dense stellar systems lie at the interface between dynamics, stellar evolution, and galaxy formation, and they provide us with an ideal;

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From Luminous Hot Stars to Starburst Galaxies

connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book;

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Cambridge Astrophysics

connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book;

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Active Ob Stars (Iau S272)

and graduate students, this volume will appeal to all those interested in extreme physical processes as tools to study structure evolution and;

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The Feedback Pendulum

different phases of education, including: the evolution of feedback over time; pre-school feedback; primary and secondary school feedback;

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The Multi-Messenger Astrophysics of the Galactic Centre (IAU S322)

The Galactic Centre represents a unique and extreme environment in the Galaxy. It hosts the Milky Way's supermassive black hole, its most;

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