This book collects a wide variety of astrophysical phenomena ranging from cosmology and galaxy formation to planet formation and organic matter that could be successfully tackled and in fact revolutionized by large millimetre array radioastronomy. The book is well balanced in presenting theoretical and observational studies and also some analysis on future strategies concerning the cooperation of various instruments. This book summarizes the exciting science ranging from the most distant and earliest galaxies to the chemistry of star and planet formation that will become accessible with these new instruments.
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The next major step in millimetre astronomy, and one of the highest-priority items in radio astronomy today, is a very large millimetre array. It will be the millimetre counterpart of the Hubble Space telescope and the new optical telescopes currently under construction, such as ESOs Very Large Telescope. As such it will produce a wide range of important scientific results in all areas of modern astrophysics, particularly cosmology and the origins of galaxies, stars, and planets. This book summarizes the exciting science that will become possible, ranging from the most distant and earliest galaxies to the chemistry and physics of star and planet formation. There are also a number of papers on the European concept and project for a large millimetre array in the southern hemisphere.
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