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Why Build Stellar Interferometers?
Harold A. McAlister (Georgia State University)
Abstract:
Optical interferometry presents high levels of technical challenge and
scientific payoff. The challenge lies in the very strict performance
requirements that must propagate through a number of complex subsystems
and the continuing development of beam combination schemes that will
yield images of relatively complex objects. The payoff, of course, is in
the science. There will be a tremendous return in fundamental
astrophysical data in impressive degrees of quantity and quality.
Optical images with milliarcsecond resolution of stars in formation or
in interaction whet everyone's scientific appetite. The future of the
field of ground-based O/IR interferometry will be determined to a large
extent over the next decade by the success (or dare one say failure) of
the current generation of instruments. If the return meets our
expectations, one can envision a future array capable of
sub-milliarcsecond imaging of cosmological objects.
Viewgraphs PDF 312k Bytes.
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Caltech 1999
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2001 | CfA 2002
Course Notes from the 2002 Michelson Interferometry Summer School
Smithsonian Astrophysical Observatory, Cambridge Massachusetts, June 24-28, 2002
Edited by P.R. Lawson (JPL), MS 301-451 Jet Propulsion Laboratory
Pasadena, California, 91109
Last Updated 9 February 2004
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