On the Near – Infrared Size of
نویسندگان
چکیده
Near–infrared (2.2 μm) long baseline interferometric observations of Vega are presented. The stellar disk of the star has been resolved, and the data have been fitted with a limb darkened stellar Jet Propulsion Laboratory, California Institute of Technology, MS 171-113, 4800 Oak Grove, Pasadena, CA 91109 Department of Physics & Astronomy, University of Wyoming, Laramie, WY 82071-3905
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