The radio-FIR correlation: Is MHD turbulence the cause?

Publications of the Astronomical Society of Australia

Volumn 20, Issue 3, 2003, Pages 252-256

  Groves, Brent A ^a   Cho, Jungyeon ^b   Dopita, Michael ^a   Lazarian, Alex ^b  

^a AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^b UNIVERSITY OF WISCONSIN MADISON   (United States)

Author keywords

Infrared: galaxies; MHD; Radio continuum: galaxies; Turbulence

Indexed keywords

EID: 0142100535     PISSN: 14486083     EISSN: 14486083     Source Type: Journal    
DOI: 10.1071/AS03016     Document Type: Article

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