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Paper: Search for Hidden Turbulent Gas through Interstellar Scintillation
Volume: 480, Structure and Dynamics of Disk Galaxies
Page: 263
Authors: Moniez, M.; Ansari, R.; Habibi, F.; Rahvar, S.
Abstract: 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 the perspectives of detection.
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