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.
General
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