
TY  - JOUR
A1  - Groves, Brent A. 
A1  - Cho, Jungyeon 
A1  - Dopita, Michael 
A1  - Lazarian, Alex 
T1  - The Radio&#8211;FIR Correlation: Is MHD Turbulence the Cause?
JF  - Publications of the Astronomical Society of Australia
JO  - Publ. Astron. Soc.  Aust.
Y1  - 2003
VL  - 20
IS  - 3
SP  - 252
EP  - 256
KW  - MHD &#8212; turbulence &#8212; infrared: galaxies &#8212; radio continuum: galaxies
UR  - https://doi.org/10.1071/AS03016 
N2  - The radio&#8211;far infrared correlation is one of the tightest correlations found in astronomy. Many of the models explaining this correlation rely on the association of global magnetic field strength with gas density. In this letter we put forward that the physical reason for this association lies within the processes of magnetohydrodynamic turbulence. 
ER  -

