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Search for Turbulent Gas through Interstellar Scintillation
Published online by Cambridge University Press: 20 April 2012
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 consider its potential.
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- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 7 , Symposium S285: New Horizons in Time-Domain Astronomy , September 2011 , pp. 376 - 378
- Copyright
- Copyright © International Astronomical Union 2012