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Techniques of mm/sub-mm Interferometry in Star Formation

Published online by Cambridge University Press:  23 September 2016

Anneila I. Sargent
Anneila I. Sargent*
Affiliation:
California Institute of Technology, MS 105-24, Pasadena, California 91125

Abstract

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Since the earliest stages of star formation occur deep in clouds of gas and dust, they are hidden from optical view. Nevertheless, infrared and millimeter wavelength observations over the last twenty years have enabled increasingly detailed studies of the processes involved in stellar birth. High resolution, aperture synthesis imaging of the millimeter-wave radiation from dust and molecular gas in star-forming clouds has proven particularly effective. On the other hand, there can be pitfalls to be avoided in the use of mm/sub-mm interferometry techniques. Here, we consider what has been learned from currently-operating mm interferometers and the potential of the next generation of arrays.

Type
Part 2: From Molecular Clouds to Protostellar Cores
Information
Symposium - International Astronomical Union , Volume 221: Star Formation at High Angular Resolution , 2004 , pp. 19 - 28
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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