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Non-ballistic motion and precessing helical trajectory in quasar NRAO 150

Non-ballistic motion and precessing helical trajectory in quasar NRAO 150

作     者:Shan-Jie Qian 

作者机构:National Astronomical ObservatoriesChinese Academy of Sciences 

出 版 物:《Research in Astronomy and Astrophysics》 (天文和天体物理学研究(英文版))

年 卷 期:2016年第16卷第1期

页      面:175-189页

核心收录:

学科分类:07[理学] 070401[理学-天体物理] 0704[理学-天文学] 

主  题:radio continuum: galaxies    galaxies: jets    galaxies: kinematics    galaxies: individual(quasar NRAO 150) 

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 *** 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 superluminal 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.

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