Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Fan, Zhonghui"'
Autor:
Wu, Jian-Chun, Gao, Shuobin, Li, Xiaowei, Zhou, Haitao, Gao, Hongquan, Hu, Jinlong, Fan, Zhonghui, Liu, Yunjian
Publikováno v:
In Journal of Colloid And Interface Science May 2024 661:1025-1032
We investigate the electron energy distributions (EEDs) and the acceleration processes in the jet of Mrk 421 through fitting the spectral energy distributions (SEDs) in different active states in the frame of a one-zone synchrotron self-Compton (SSC)
Externí odkaz:
http://arxiv.org/abs/1301.6476
Autor:
Fan, Zhonghui, Liu, Siming
Stochastic acceleration of charged particles due to their interactions with plasma waves may be responsible for producing superthermal particles in a variety of astrophysical systems. This process can be described as a diffusion process in the energy
Externí odkaz:
http://arxiv.org/abs/1112.6316
The quasi-simultaneous multi-wavelength emission of TeV blazar 3C 66A is studied by using a one-zone multi-component leptonic jet model. It is found that the quasi-simultaneous spectral energy distribution (SED) of 3C 66A can be well reproduced, espe
Externí odkaz:
http://arxiv.org/abs/1011.1537
Publikováno v:
ApJ 735 (2011) 120
Emission mechanisms of the shell-type supernova remnant (SNR) RX J1713.7-3946 are studied with multi-wavelength observational data from radio, X-ray, GeV $\gamma$-ray to TeV $\gamma$-ray band. A Markov Chain Monte Carlo method is employed to explore
Externí odkaz:
http://arxiv.org/abs/1011.0145
(Aims.) SNR RX J1713.7-3946 is perhaps one of the best observed shell-type supernova remnants with emissions dominated by energetic particles accelerated near the shock front. The nature of the TeV emission, however, is an issue still open to investi
Externí odkaz:
http://arxiv.org/abs/1007.0796
In the leptonic scenario for TeV emission from a few well-observed shell-type TeV supernova remnants (STTSNRs), very weak magnetic fields are inferred. If fast-mode waves are produced efficiently in the shock downstream, we show that they are viable
Externí odkaz:
http://arxiv.org/abs/0909.3349
Publikováno v:
Res.Astron.Astrophys.9:1192-1204,2009
We have collected all available spectra and photometric data from SDSS catalogue for bright AGNs complied from the first three months of the Fermi large area telescope all-sky survey. Based on the 106 high-confidence and 11 low-confidence association
Externí odkaz:
http://arxiv.org/abs/0906.3373
Publikováno v:
Astrophys.J.646:8-15,2006
There is clear evidence that the $\gamma$-ray emission from active galactic nuclei (AGNs) is attributed to the inverse Compton scatterings in the relativistic blobs near the massive black holes. If the soft seed photons are from the regions outside t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0604019
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