Ground-based optical interferometry

Details Ground-based optical interferometry Ground-based optical interferometry

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.273..119r&link_type=abstract

In ESA, ESA Workshop on Optical Interferometry in Space p 119-125 (SEE N88-10613 01-74)

Astronomy and Astrophysics

Astronomy

Astronomical Observatories, Interferometry, Space Observations (From Earth), Speckle Patterns, Synthetic Apertures, Telescopes

Scientific paper

Progress in ground based multitelescope interferometry is reviewed. Interferometric methods progressed rapidly, leading to image reconstruction of numerous extended sources. Phase closure is demonstrated. Several two-telescope systems obtained fringes and results. Automation of a two-telescope interferometer is demonstrated. Scientific results include image reconstructions, accurate angular diameters, spatio-spectrally resolved emission lines from a Be star, asteroid shapes and maps, satellite diameters, measures of shells around young and old stars, and detections and measurement of binary and multiple stars.

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