Abstract
During the past three years we have been using the computer controlled 2.3 meter telescope at the Wyoming Infrared Observatory to generate infrared images. Brief descriptions of the technique have been given by Grasdalen et. al. (1980) and Herzog et. al. (1980). The technique has been successfully applied to imaging regions of star formation (Hackwell et. al. 1982, Gehrz et. al. 1982) planetary nebulae (Bentley, 1982) and planets (Grasdalen et. al. 1983).
© 1983 Optical Society of America
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