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A Plasmon Driven Bowshock Model for the Narrow Line Region of NGC 5929
1989
International Astronomical Union Colloquium
Close links appear to exist between the optical narrow line region (NLR) in Seyfert galaxies and the nuclear non-thermal radio emission. Both occur on similar scales (~ 102—103pc), and correlations have been found between the 21 cm radio power and both the [OIII] λ5007Åluminosity and linewidth (de Bruyn & Wilson 1978; Whittle 1985). Approximate balance appears to exist between the thermal pressure of the NLR gas and the relativistic and magnetic pressure of the radio components (de Bruyn
doi:10.1017/s0252921100024106
fatcat:akgs3wztmvgc5iyo4nblldjowe