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Comprehensive and robust analysis of galaxies found throughout cosmic time provides the means to probe the underlying characteristics of our Universe. Coupling observations and theory, spectral energy...
We have analyzed the new Rossi X-ray Timing Explorer Proportional Counter Array data of the atoll neutron star (NS) low-mass X-ray binary (LMXB) system XB 1254-690. The colour-colour diagram shows tha...
We have produced the next generation of quasar spectral energy distributions (SEDs), essentially updating the work of Elvis et al. (1994) by using high-quality data obtained with several space and gro...
We report the observation of nearest quasar 3C273 made with LASE instrument on November 20th, 1998 as a part of our continuing programme of balloon borne hard X-ray observations in the 20–200 keV b...
The attempts at unified model fitting to explain the spectral variations in Cyg X-3 suggest equally probable fits with a combination of an absorbed blackbody and a separately absorbed power law with...
The influence of gravitational microlensing on the X-ray spectral line profiles originated from a relativistic accretion disc has been studied. Using a disc model, we show that microlensing can indu...
The influence of gravitational microlensing on the X-ray spectral line profiles originated from a relativistic accretion disc has been studied. Using a disc model, we show that microlensing can indu...
The Gamma-ray Bright Blazars: Spectral Properties in X-Rays and Gamma-Rays           font style='font-size:12px;'> 2007/7/28
期刊信息 篇名 The Gamma-ray Bright Blazars: Spectral Properties in X-Rays and Gamma-Rays 语种 英文 撰写或编译 撰写 作者 戴本忠、张力 第一作者单位 云南大学物理学 刊物名称 PASJ 页面 939-945 出版日期 2003年 10月 日 文章标识(ISSN) 0004-6264 相关项目 γ噪blazar天体快速光...

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