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Star Formation by Future Millimetre and Radio Interferometers

Published online by Cambridge University Press:  23 September 2016

Lewis B.G. Knee
Lewis B.G. Knee*
Affiliation:
Dominion Radio Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council, Box 248, Penticton, BC, V2A 6J9, Canada

Abstract

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The Low Frequency Array (LOFAR), the Atacama Large Millimetre Array (ALMA), and the Square Kilometre Array (SKA) will be the largest and most capable aperture synthesis facilities of the next few decades. The advances in our knowledge of star formation that ALMA will permit are well known to the star formation community, but the potential of the SKA has so far attracted less attention. I will outline the star formation science cases of these upcoming facilities, with an emphasis on the SKA.

Type
Part 10: The Future of Star Formation At High Angular Resolution
Information
Symposium - International Astronomical Union , Volume 221: Star Formation at High Angular Resolution , 2004 , pp. 461 - 470
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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