activity
20072013
most citedEmitting electrons spectra and acceleration processes in the jet of Mrk 421: from low state to giant flare state

63 citations · 253 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2013★ 63 cited

Emitting electrons spectra and acceleration processes in the jet of Mrk 421: from low state to giant flare state

Dahai Yan, Li Zhang, Qiang Yuan +2

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 a…

astro-ph.HE2011

Stochastic Electron Acceleration in SNR RX J1713.7-3946

Zhonghui Fan, Siming Liu

Stochastic acceleration of charged particles due to their interactions with plasma waves may be responsible for producing superthermal particles in a variety of astrophysical syste…

astro-ph.HE2010★ 4 cited

Multi-wavelength emission from 3C 66A: clues on its redshift and gamma-ray emission location

Dahai Yan, Zhonghui Fan, Yao Zhou +1

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 spe…

astro-ph.HE2010★ 55 cited

Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946

Qiang Yuan, Siming Liu, Zhonghui Fan +2

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 -ray to TeV -ray ban…

astro-ph.HE2010★ 19 cited

Lepton Models for TeV Emission from SNR RX J1713.7-3946

Zhonghui Fan, Siming Liu, Qiang Yuan +1

(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…

astro-ph.HE2009★ 24 cited

Stochastic Electron Acceleration in the TeV Supernova Remnant RX J1713.7-3946: The High-Energy Cut-off

Zhonghui Fan, Siming Liu, Christopher L. Fryer

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 produ…