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Tenth Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe (UCLA Dark Matter 2012), Marina del Rey : United States (2012)
Search for Turbulent Gas through Interstellar Scintillation
Marc Moniez1, R. Ansari1, F. Habibi1, 2, S. Rahvar2

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.
1 :  LAL - Laboratoire de l'Accélérateur Linéaire
2 :  Sharif University of Technology, Dept. of Physics
Energie Noire
Physique/Astrophysique/Astrophysique galactique

Planète et Univers/Astrophysique/Astrophysique galactique
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moniez-DM2012-OSER.pdf(483.7 KB)
moniez-DM2012-OSER.ps(911.5 KB)