ALMA from the User Perspective: Galactic

Details ALMA from the User Perspective: Galactic ALMA from the User Perspective: Galactic

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21731704w&link_type=abstract

American Astronomical Society, AAS Meeting #217, #317.04; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

ALMA will be "transformative" for studies of cool components of the Galaxy, in particular the molecular gas and dust in the immediate vicinity of young or evolved stars where arcsecond or higher resolution will be especially valuable to probe structure, dynamics, and chemistry. At the start of Early Science scheduled for 2011, the subset of available ALMA antennas already will provide spectral line and continuum sensitivity and imaging capabilities that exceed any of the existing millimeter arrays. Using examples from star-forming regions and circumstellar disks, I will illustrate how a prospective ALMA user can realize the fantastic potential of this new facility in the Early Science stage and beyond.

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