Search for Turbulent Gas through Interstellar Scintillation

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.
Type de document :
Communication dans un congrès
D. Cline. Tenth Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe (UCLA Dark Matter 2012), Feb 2012, Marina del Rey, United States. Springer, 148, pp.45-49, 2013, Springer Proceedings In Physics. <10.1007/978-94-007-7241-0_6>


http://hal.in2p3.fr/in2p3-00723051
Contributeur : Marc Moniez <>
Soumis le : mercredi 22 août 2012 - 19:16:03
Dernière modification le : lundi 13 octobre 2014 - 15:43:25
Document(s) archivé(s) le : vendredi 23 novembre 2012 - 02:20:38

Fichiers

moniez-DM2012-OSER.pdf
Fichiers produits par l'(les) auteur(s)

Identifiants

Collections

LAL

Citation

Marc Moniez, R. Ansari, F. Habibi, S. Rahvar. Search for Turbulent Gas through Interstellar Scintillation. D. Cline. Tenth Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe (UCLA Dark Matter 2012), Feb 2012, Marina del Rey, United States. Springer, 148, pp.45-49, 2013, Springer Proceedings In Physics. <10.1007/978-94-007-7241-0_6>. <in2p3-00723051>

Exporter

Partager

Métriques

Consultations de
la notice

110

Téléchargements du document

70