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Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237)
New stars form in the dense turbulent gas clouds of galaxies. A wide variety of processes, with scales ranging from the size of a galaxy to the size of an individual star, drive …
Waves and Oscillations in the Solar Atmosphere (IAU S247)
IAU Symposium 247 addresses the latest discoveries on magnetic waves and oscillations, observed recently in the atmosphere of the Sun. The energy sources which maintain the …
Formation, Evolution, and Survival of Massive Star Clusters (IAU S316)
Massive star clusters are invaluable bridges connecting the interstellar medium, star formation and evolution, the evolution of galaxies, and cosmology. These very complex systems …
Planetary Nebulae (IAU S283)
Planetary nebulae play a key role in stellar evolution as an important fraction of stellar matter in the Universe goes through the asymptotic giant branch and planetary nebula …
Solar and Astrophysical Dynamos and Magnetic Activity (IAU S294)
Global magnetic fields in planets, in the Sun and other stars, in spiral galaxies and galaxy clusters are believed to be generated and maintained by a hydromagnetic dynamo, a …
Binary Stars as Critical Tools and Tests in Contemporary Astrophysics (IAU S240)
IAU Symposium 240, held in conjunction with the 26th General Assembly of the International Astronomical Union, highlights the latest advances in the field of binary and multiple …
Formation and Evolution of Galaxy Outskirts (IAU S321)
The borders between galaxies and the almost empty intergalactic medium are ill-defined regions where gas struggles to form stars. The proceedings of IAU Symposium 321 summarize our …