Gamma-ray emission from massive stars interacting with active galactic nuclei jets

被引:49
作者
Araudo, A. T. [1 ]
Bosch-Ramon, V. [2 ]
Romero, G. E. [3 ,4 ]
机构
[1] Univ Nacl Autonoma Mexico, Ctr Radioastron & Astrofis, Morelia 58089, Michoacan, Mexico
[2] Univ Barcelona, Dept Astron & Meteorol, E-08028 Barcelona, Spain
[3] Inst Argentino Radioastron, Buenos Aires, DF, Argentina
[4] Univ Nacl La Plata, Fac Ciencias Astron &Geofis, RA-1900 La Plata, Argentina
关键词
radiation mechanisms: non-thermal; stars: early-type; galaxies: active; gamma-rays: theory; HIGH-ENERGY EMISSION; BLACK-HOLES; SYNCHROTRON-RADIATION; MODELS; ACCELERATION; GALAXIES; ACCRETION; POWER; BASE;
D O I
10.1093/mnras/stt1840
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, these stars can interact with the relativistic jets launched by the supermassive black hole. In this work, we study the interaction of early-type stars with relativistic jets in active galactic nuclei. A bow-shaped double-shock structure is formed as a consequence of the interaction of the jet and the stellar wind of each early-type star. Particles can be accelerated up to relativistic energies in these shocks and emit high-energy radiation. We compute, considering different stellar densities of the galactic core, the gamma-ray emission produced by non-thermal radiative processes. This radiation may be significant in some cases, and its detection might yield valuable information on the properties of the stellar population in the galaxy nucleus, as well as on the relativistic jet. This emission is expected to be particularly relevant for nearby non-blazar sources.
引用
收藏
页码:3626 / 3639
页数:14
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