Jet in jet in M87

被引:12
|
作者
Sob'yanin, Denis Nikolaevich [1 ,2 ]
机构
[1] Russian Acad Sci, PN Lebedev Phys Inst, IE Tamm Div Theoret Phys, Leninskii Prospekt 53, Moscow 119991, Russia
[2] State Univ, Moscow Inst Phys & Technol, Inst Skii Pereulok 9, Dolgoprudnyi 141701, Russia
基金
俄罗斯科学基金会;
关键词
galaxies: individual: M87; galaxies: jets; SUPERMASSIVE BLACK-HOLE; DOUBLE RADIO-SOURCES; ACCRETION DISK; WINDS; ROTATION; DRIVEN; ENERGY; GALAXY; SPACE; MODEL;
D O I
10.1093/mnras/stx1767
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
New high-resolution Very Long Baseline Interferometer observations of the prominent jet in the M87 radio galaxy show a persistent triple-ridge structure of the transverse 15-GHz profile with a previously unobserved ultra-narrow central ridge. This radio structure can reflect the intrinsic structure of the jet, so that the jet as a whole consists of two embedded coaxial jets. A relativistic magnetohydrodynamic model is considered in which an inner jet is placed inside a hollow outer jet and the electromagnetic fields, pressures and other physical quantities are found. The entire jet is connected to the central engine that plays the role of a unipolar inductor generating voltage between the jets and providing opposite electric currents, and the charge neutrality and current closure together with the electromagnetic fields between the jets can contribute to the jet stabilization. The constant voltage is responsible for the similar widening laws observed for the inner and outer jets. This jet-in-jet structure can indicate simultaneous operation of two different jet-launching mechanisms, one relating to the central supermassive black hole and the other to the surrounding accretion disc. An inferred magnetic field of 80 G at the base is sufficient to provide the observed jet luminosity.
引用
收藏
页码:4121 / 4127
页数:7
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