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Search for hidden 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 of detection.
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http://hal.in2p3.fr/in2p3-00855450
Contributor : Sabine Starita <>
Submitted on : Thursday, August 29, 2013 - 2:28:37 PM
Last modification on : Wednesday, September 16, 2020 - 4:23:36 PM
Long-term archiving on: : Monday, December 2, 2013 - 8:54:24 AM

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  • HAL Id : in2p3-00855450, version 1
  • ARXIV : 1308.6472

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IN2P3 | LAL | CNRS

Citation

M. Moniez, R. Ansari, F. Habibi, S. Rahvar. Search for hidden turbulent gas through interstellar scintillation. Structure and dynamics of disk galaxies, Aug 2013, Petit Jean Mountain, United States. pp.263. ⟨in2p3-00855450⟩

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