“School of Astronomy”
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Paper IPM / Astronomy / 12883 | ||||||||||||||||||||||||||
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Stars twinkle because their light propagates through the atmosphere. The same phenomenon is expected when the light of remote stars crosses a Galactic-disk or halo-refractive medium such as a molecular cloud. We present the promising results of a test performed with the ESO-NTT, and consider its potential.
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