Magnetic fields and ionized gas in the inner galaxy: An outer scale for turbulence and the possible role of H II regions

Astrophysical Journal

Volumn 609, Issue 2 I, 2004, Pages 776-784

  Haverkorn, M ^a   Gaensler, B M ^a   McClure Griffiths, N M ^b   Dickey, John M ^c   Green, A J ^d  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b CSIRO   (Australia)

^c University of Minnesota   (United States)

^d UNIVERSITY OF SYDNEY   (Australia)

Author keywords

Galaxy: structure; H II regions; ISM: structure; Radio continuum: ISM; Techniques: polarimetric; Turbulence

Indexed keywords

EID: 3242767709     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/421341     Document Type: Article

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