Non-ballistic motion and precessing helical trajectory in quasar NRAO 150
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摘要:
NRAO 150 is a very special radio quasar in which prominent non-ballistic superluminal motion has been observed in its inner-jet region.We apply model-fittings to the kinematics of the superluminal knots (trajectory,distance from the core and apparent velocity) in terms of a helical precessing jet-nozzle model.Five cases are considered in which the angle between the jet axis and the line of sight is assumed to be 6°,3°,1°,0.6° and 0.12°,respectively.It is shown that the supeduminal components have intrinsic acceleration in the innermost regions ((~) 0.2 mas from the core).The phenomenon of precessing nozzle/trajectory can be understood on the basis of relativistic magnetohydrodynamic theories for relativistic jets.