Zobrazeno 1 - 10
of 8 176
pro vyhledávání: '"Hai, Ming"'
Autor:
Chen, Xiao-Bin, Wang, Kai, Huang, Yi-Yun, Zhang, Hai-Ming, Xi, Shao-Qiang, Liu, Ruo-Yu, Wang, Xiang-Yu
The supersonic flow motions associated with infall of baryonic gas toward sheets and filaments, as well as cluster mergers, produces large-scale shock waves. The shocks associated with galaxy clusters can be classified mainly into two categories: int
Externí odkaz:
http://arxiv.org/abs/2412.02436
Autor:
Hu, Hai-Ming, Huang, Guang-Shun
One method to determine the characteristic parameters of a hadron production source is to measure Bose-Einstein correlation functions. In this paper, we present fundamental concepts and formulas related to Bose-Einstein correlations, focusing on the
Externí odkaz:
http://arxiv.org/abs/2410.06503
Autor:
Tao, Ze-Hua, Lavor, Icaro R., Dong, Hai-Ming, Chaves, Andrey, Neilson, David, Milosevic, Milorad V.
We demonstrate chiral propagation of plasmon polaritons and show it is more efficient and easier to control than the recently observed chiral shear phonon polaritons. We consider plasmon polaritons created in an anisotropic two-dimensional (2D) mater
Externí odkaz:
http://arxiv.org/abs/2409.11066
Autor:
Li, Jia-Xuan, Hu, Xin-Ke, Lian, Ji-Shun, Yu, Yu-Wei, Deng, Wei, Liu, Kuan, Zhang, Hai-Ming, Chen, Liang, Zhang, Jin
Pictor A is a $\gamma$-ray emitting radio galaxy and has a bright hotspot called WHS, located $\sim$4 arcmin away from the nucleus. In this letter, we present an analysis of its 16-year Fermi-LAT data and report the first Imaging X-ray Polarimetry Ex
Externí odkaz:
http://arxiv.org/abs/2407.21277
We investigate the asymmetric propagation of 100 TeV electrons (whose radiation mainly concentrates on 20--30 TeV) in turbulent magnetic fields around pulsars, using GPU-accelerated simulations to explore their trajectories and interactions within pu
Externí odkaz:
http://arxiv.org/abs/2407.02829
The study of extended $\gamma$-ray sources usually assumes symmetric diffusion of cosmic rays. However, recent observations of multiple sources near single pulsars and significant offsets between TeV halo centroids and their parent pulsars suggest th
Externí odkaz:
http://arxiv.org/abs/2407.02478
Publikováno v:
JHEAP, 2024, 43: 171-177
Nova shocks behave like scaled-down supernova remnant shocks with a lifetime of only a few weeks or months, thereby providing a unique opportunity to study the dynamics of non-relativistic shocks as well as the shock acceleration physics. Recently, G
Externí odkaz:
http://arxiv.org/abs/2405.01257
Autor:
Lian, Ji-Shun, Li, Jia-Xuan, Hu, Xin-Ke, Gan, Ying-Ying, Wu, Tan-Zheng, Zhang, Hai-Ming, Zhang, Jin
NGC 4278, a Low-luminosity active galactic nucleus (AGN), is generally classified as a low-ionization nuclear emission line region (LINER). Recently, it has been reported to be associated with a very high energy $\gamma$-ray source 1LHAASO J1219+2915
Externí odkaz:
http://arxiv.org/abs/2405.00347
The radio galaxy PKS 1007+142 is classified as a compact steep-spectrum source (CSS) and belongs to the class of young Active Galactic Nuclei (AGNs). In this paper, we investigate the $\gamma$-ray emission from this CSS by conducting a comprehensive
Externí odkaz:
http://arxiv.org/abs/2404.16373
We report on the detection of extended $\gamma$-ray emission from lobes in the radio galaxy NGC 6251 using observation data of Fermi Large Area Telescope (Fermi-LAT). The maximum likelihood analysis results show that a radio morphology template provi
Externí odkaz:
http://arxiv.org/abs/2402.04591