Low-Mach-number turbulence in interstellar gas revealed by radio polarization gradients

B M Gaensler1, M Haverkorn, B Burkhart

  • 1Sydney Institute for Astronomy, School of Physics, The University of Sydney, New South Wales 2006, Australia. bryan.gaensler@sydney.edu.au

Nature
|October 7, 2011
PubMed

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