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Low-Metallicity Star Formation (Iau S255)

events in low-metallicity environments; dust and gas as seeds for metal-poor star formation; metal-poor initial mass functions, stellar evolution;

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Dwarf Galaxies (IAU S344)

, with sections dedicated to: Local Group dwarf galaxies; the interstellar medium and star formation in dwarfs; metallicity, massive stars, and;

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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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Computational Star Formation (Iau S270)

in the fields of interstellar gas dynamics, star formation and galactic dynamics. It includes numerical techniques for modeling physical;

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Star-Disk Inter In Young Star (IAU S243)

Stars form surrounded by a circumstellar disk which is thought to be the cradle of planets. IAU Symposium 243 highlights the latest;

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Massive Stars As Cosmic Engines (Iau S250)

massive stars at low metallicity are also included.;

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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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From Interacting Binaries To Exoplanets (Iau S282)

In IAU Symposium 282, members of the exoplanet and binary star communities unite for the first time to discuss the state-of-the-art;

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The Labyrinth of Star Formation

aspects of theoretical and observational star formation: low-mass star formation; young circumstellar discs; computational methods; triggered star;

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Cambridge Contemporary Astrophysics

stars we can gain valuable insights into how metals change the formation and evolution of stars, and explain the extraordinary massive star;

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Molecular Gas, Dust, And Star Formation In Galaxies (Iau S29

related topics including the initial conditions for star formation, observational tracers of star formation and interstellar conditions, and;

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The Metal-Rich Universe

stars we can gain valuable insights into how metals change the formation and evolution of stars, and explain the extraordinary massive star;

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The Properties of Star-Forming Galaxies at z~2

through IR photometry, we examine the galaxies' star formation properties, dynamical masses and velocity dispersions, spatially resolved;

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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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Laboratory Astrophysics (IAU S350)

today. Five major topics are covered, spanning from star- and planet-formation through stellar populations to extragalactic chemistry and dark;

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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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Proceedings of the International Astronomical Union Symposia and Colloquia

techniques, before looking at the physics of gas giant atmospheres and close-in stars. The topics of planet formation, migration and the dynamical;

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Galactic Bulges

This book contains the proceedings of the first large IAU Symposium dedicated to the bulges of spiral galaxies. Detailed attention is paid;

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High-mass X-ray Binaries (IAU S346)

IAU Symposium 346. Taking an interdisciplinary approach, it includes reviews on massive star winds and HMXB donors, Be Stars in the X-ray;

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Physics Of Sun And Star Spots (Iau S273)

irradiance. Combined study of the spots on the Sun and on other stars provides a greater understanding of sunspot formation and behaviour on a long;

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

concentrated dense gas reservoir and its most extreme star-formation environment. The Galactic Centre is therefore our nearest analogue to both an;

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

, and jets, which heat and perhaps remove entirely the interstellar medium of the host galaxy, effectively shutting down star formation. These;

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Galaxy Evolution and Feedback across Different Environments (IAU S359)

center fuelled to become an AGN? What is the main physical mechanism that quenches star formation? How powerful are the stellar and AGN feedback;

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Starburst Galaxies

A major fraction of star formation in the universe occurs in starbursts. These regions of particularly rapid star formation are often;

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Introduction To Star Formation

Guiding the reader through all the stages that lead to the formation of a star such as our Sun, this advanced textbook provides students;

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Living around Active Stars (IAU S328)

habitable exoplanets. IAU Symposium 328 brings together diverse, interdisciplinary reviews and research papers which address the themes of star;

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Fine Structure and Dynamics of the Solar Photosphere (IAU S327)

unprecedented temporal and spatial resolutions. This volume includes recent results in solar physics research presented at the IAU Symposium 327, the;

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