Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989tidt.work..283t&link_type=abstract
In NASA, Ames Research Center, Proceedings of the Third Infrared Detector Technology Workshop p 283-293 (SEE N90-21313 14-35)
Astronomy and Astrophysics
Astronomy
Infrared Astronomy, Interferometers, Speckle Interferometry, Stars, Stellar Spectra, Cameras, Power Spectra
Scientific paper
Preliminary two-dimensional speckle interferometry results of HL Tau were found to be qualitatively similar to those found with one-dimensional slit scanning techniques; results consist of a resolved component (approximately 0.7 arcsec in size) and an unresolved component. Researchers are currently reducing the rest of the data (taken on three different telescopes and at three different wavelengths) and are also exploring other high resolution methods like the shift and add technique and selecting only the very best images for processing. The availability of even better two-dimensional arrays within the next couple of years promises to make speckle interferometry and other high resolution techniques very powerful and exiting tools for probing a variety of objects in the subarcsec regime.
Harvey Paul Michael
Tollestrup Eric V.
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