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Optical/IR Interferometry: Star Formation at sub-AU Scales

Published online by Cambridge University Press:  23 September 2016

Peter Tuthill
Peter Tuthill*
Affiliation:
Astronomy Department, School of Physics, University of Sydney, N.S.W. 2006, Australia

Abstract

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Intermediate to late stages of star formation are characterized by rising infrared and visible luminosities, with much of the most interesting physics concentrated in the inner regions within the immediate vicinity of the central protostar(s). Long-baseline optical and infrared interferometry is ideally suited to study of such bright, compact structures. Contributions from presently operational arrays, which are capable of resolving the brightest few dozen, will be reviewed. These results presage the potential for further dramatic advances in our understanding of star formation with observations from more advanced instruments now being built.

Type
Part 9: The Influence of Planets During Star Formation
Information
Symposium - International Astronomical Union , Volume 221: Star Formation at High Angular Resolution , 2004 , pp. 433 - 440
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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