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The Future of High Angular Resolution Star and Planet Formation Science in the Optical/Infrared

Published online by Cambridge University Press:  23 September 2016

Lynne A. Hillenbrand
Lynne A. Hillenbrand*
Affiliation:
California Institute of Technology, Pasadena, CA 91125

Abstract

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This presentation summarizes how some of the most pressing questions in the field of star and planet formation can be addressed by high angular resolution optical/infrared capabilities, and how many of these capabilities will in fact be available with realization of the space and ground facilities currently being planned for the 2005-2020 time frame.

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. 471 - 479
Copyright
Copyright © Astronomical Society of the Pacific 2004