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Titlebook: Science with the Atacama Large Millimeter Array:; A New Era for Astrop Rafael Bachiller,José Cernicharo Conference proceedings 2008 Springe

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Star and planet-formation with ALMA: an overview,led imaging of the collapse of pre-stellar cores and measuring the accretion rate of matter onto deeply embedded protostars, to unravelling the chemistry and dynamics of high-mass star-forming clusters and high-spatial resolution studies of protoplanetary disks down to the 1 AU scale.
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Interstellar deuteroammonia,ll as .-deuterated ammonia and methanol. We review the current understanding of depletion and deuteration processes in cold, dense interstellar medium (ISM) and discuss the utility of deuteroammonia as a tracer of the physical conditions and kinematics of cold, dense gas.
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High resolution submillimeter observations of massive protostars, evolutionary stages coexisting in close proximity. In the presence of such complexity and multiplicity of sources, these data suggest that the interpretation of diagnostics such as kinematic velocity gradients and temperatures that are strongly dependent on spatial resolution should be approached cautiously.
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APEX and ATCA observations of the southern hot core G327.3-0.6 and its environs,ith cm continuum observations, the data reveal like pearls on a string several stages of massive star formation, with likely the youngest stages hiding in the cold N.H. cores analysed with a multilevel study of the APEX and ATCA observations.
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prospects with such a unique facility.Provides the science c.Currently under construction in the Andean Altiplano, Northern Chile, the Atacama Large Millimeter Array (ALMA) is the most ambitious astronomy facility under construction. ALMA is a radio interferometer composed of 54 antennas of 12 m dia
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