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| HAL : in2p3-00723051, version 1 |
| arXiv : 1208.6377 |
| Fiche détaillée |  Récupérer au format |
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| Tenth Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe, Los-Angeles : États-Unis (2012) |
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| Search for Turbulent Gas through Interstellar Scintillation |
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| Marc Moniez1R. Ansari1F. Habibi1, 2S. Rahvar2 |
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| (07/08/2012) |
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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 the perspectives. |
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| 1 : | LAL - Laboratoire de l'Accélérateur Linéaire |
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| 2 : | Sharif University of Technology, Dept. of Physics |
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| Thème(s) | : | Physique/Astrophysique/Astrophysique galactique Planète et Univers/Astrophysique/Astrophysique galactique |
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| Liste des fichiers attachés à ce document : | ||||||||||
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| in2p3-00723051, version 1 | |
| http://hal.in2p3.fr/in2p3-00723051 | |
| oai:hal.in2p3.fr:in2p3-00723051 | |
| Contributeur : Marc Moniez | |
| Soumis le : Mercredi 22 Août 2012, 19:16:03 | |
| Dernière modification le : Vendredi 31 Août 2012, 08:18:44 | |
