The content of astrophysical jets

被引:8
|
作者
Romero, Gustavo E. [1 ,2 ]
机构
[1] UNLP, CICPBA, CONICET, Inst Argentino Radioastron IAR, Buenos Aires, DF, Argentina
[2] Univ Nacl La Plata, Fac Ciencias Astron & Geofis, Buenos Aires, DF, Argentina
关键词
jets; black holes; magnetic fields; accretion; SUPERMASSIVE BLACK-HOLES; THICK ACCRETION DISKS; HIGH-ENERGY PARTICLES; GAMMA-RAY EMISSION; RELATIVISTIC JETS; NONTHERMAL PROCESSES; 3D SIMULATIONS; TEV EMISSION; M87; JET; FLOWS;
D O I
10.1002/asna.202113989
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Jets, collimated outflows of particles and fields, are observed in a wide variety of astrophysical systems, including Active Galactic Nuclei of various types, micro-quasars, gamma-ray bursts, and young stellar objects. Despite intensive efforts along several decades of observational and theoretical research, there are still many uncertainties and open questions related to how jets are produced and what is their composition. In this review, I offer an outline of some current views on the content and basic properties of astrophysical jets.
引用
收藏
页码:727 / 734
页数:8
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