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Cosmic masers, naturally occurring amplifiers of microwave emission from atoms and molecules in the Milky Way and other galaxies, provide important to...Lees meer
Our comprehension of the assembly and evolution of galaxies has witnessed remarkable advancements in recent years. While the Gaia spacecraft has provi...Lees meer
Near Earth Objects (NEOs), asteroids and comets, are the closest neighbors of the Earth-Moon system. They allow research not yet possible on more dist...Lees meer
IAU Symposium 356 summarises the most recent results in the field of active galaxies and active galactic nuclei (AGN). These are some of the most lumi...Lees meer
Stellar cluster research is in a dynamic state. IAU Symposium 351 (also chosen as MODEST-19, within the 'Modelling and Observing DEnse STellar systems...Lees meer
Massive star clusters are invaluable bridges connecting the interstellar medium, star formation and evolution, the evolution of galaxies, and cosmolog...Lees meer
This volume presents papers concerning astronomy education and research in developing countries presented at a special session at the IAU 26th General...Lees meer
New telescopes spanning the full electromagnetic spectrum have enabled the study of supernovae (SNe) and supernova remnants (SNRs) to advance at a bre...Lees meer
IAU Symposium 271 enhances our understanding of some of the important dynamical processes that are ubiquitous in many objects in the Universe, from st...Lees meer
All phases of stellar evolution are influenced by the presence of magnetic fields in the star's interior and close environment. IAU Symposium 302 give...Lees meer
Dwarf galaxies offer a valuable insight into the physical processes that govern galaxy formation and evolution at high redshift. These elusive stellar...Lees meer
Perseus is an outstanding case in which to study the physics of relativistic plasma and thermal gas, and the interplay between galactic nuclei and gal...Lees meer
This comprehensive collection of reviews and research reports covers the processes involved in the formation of the Sun and Earth-like planets. Specif...Lees meer
The prime parameter determining the evolution of a star is its mass. Any modification to the stellar mass has large repercussions on its evolutionary ...Lees meer
The range of phenomena that manifest at all different time and length scales and the wide range of sizes of space objects, from minor bodies in the So...Lees meer
IAU Symposium 285, New Horizons in Time-Domain Astronomy, gave a comprehensive overview of the status quo in 2011, exploring, astronomical variability...Lees meer
The rapid advance of computer capabilities over the last two decades has opened up a new field of numerical simulations in which detailed physical mod...Lees meer
At the XXIX IAU General Assembly held in Honolulu from 3-14 August 2015, the meetings known as Special Sessions and Joint Discussions were replaced by...Lees meer
IAU Symposium 269 celebrates the 400th anniversary of Galileo Galilei's discovery of the Medicean Moons, Jupiter's four largest satellites, exploring ...Lees meer
Planetary nebulae are generated when the outer layers of intermediate-mass stars are ejected during the second giant expansion after core helium burni...Lees meer
For thousands of years people have looked to the skies to better understand the universe and our place within it. Crucially it is the role of teachers...Lees meer
Until recently, black holes were often considered as exotic objects of dubious existence. In the last decade, observations have provided overwhelming ...Lees meer
Celebrating the centenary of George Ellery Hale's discovery of magnetic fields in sunspots, IAU Symposium 273 reviews the recent advances made in the ...Lees meer
The borders between galaxies and the almost empty intergalactic medium are ill-defined regions where gas struggles to form stars. The proceedings of I...Lees meer