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IAU Symposium 309 contains contributions on the timely theme of spatially and energetically resolved properties of galaxies. New technologies in 3D spectroscopy in the optical and near-infrared regimes, and radio interferometry, allow for the first time the efficient mapping of stars, gas and dust in galaxies near and far. This volume demonstrates how detailed measurements of individual objects are complemented by surveys aiming at a full census of galaxies across the local Universe. Reaching out to the limits of the Universe, the evolution of spatially resolved properties is traced throughout our whole cosmic history. In parallel with this, new computer technology and highly advanced algorithms are exploited for detailed simulations to probe the underlying physical and cosmological connections. This volume benefits astronomers and graduate students working in areas relating to galaxy formation and evolution, star formation, dust and stellar populations.
List of contents
Preface; 1. Instrumentation; 2. Nearby galaxies; 3. Feedback and environment; 4. High red-shift galaxies; Index.
Summary
IAU S309 presents contributions on the timely theme of spatially and energetically resolved properties of galaxies throughout cosmic history, including cutting-edge observational and computing technologies. This volume benefits astronomers and graduate students working in areas relating to galaxy formation and evolution, star formation, dust and stellar populations.
