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Proceedings Paper

Multiple-telescope optical interferometric array
Author(s): Harold A. McAlister; William G. Bagnuolo; W. I. Hartkopf; Allen K. Garrison
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Paper Abstract

A feasibility study of a multiple telescope array for high-spatial-resolution astronomy has been completed, and an initial design concept has been defined. The array (referred to as the CHARA array for Georgia State University's Center for High Angular Resolution Astronomy) would consist of seven 1-m-aperture telescopes in a VLA-type configuration contained within a circle of 400-m-diameter to provide a limiting resolution of 0.3 milliarcsec for stellar angular diameter measurements or 0.1 mas for binary-star measurements. The initial scientific program will be directed at the imaging of stars to determine stellar radii, masses, temperatures, distances, and surface morphology. The array is also intended to provide the means of developing techniques for the very-high-resolution imaging of a large class of objects with geometries far more complicated than those of stars and star systems.

Paper Details

Date Published: 1 August 1990
PDF: 9 pages
Proc. SPIE 1237, Amplitude and Intensity Spatial Interferometry, (1 August 1990); doi: 10.1117/12.19279
Show Author Affiliations
Harold A. McAlister, Georgia State Univ. (United States)
William G. Bagnuolo, Georgia State Univ. (United States)
W. I. Hartkopf, Georgia State Univ. (United States)
Allen K. Garrison, Georgia Tech Research Institute (United States)


Published in SPIE Proceedings Vol. 1237:
Amplitude and Intensity Spatial Interferometry
James B. Breckinridge, Editor(s)

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