Contribution to diffuse gamma-rays in the Galactic Centre region from unresolved millisecond pulsars

Diffuse gamma-rays in the Galactic Centre region have been studied. We propose that there exists a population of millisecond pulsars in the Galactic Centre, which emit GeV gamma-rays through synchrotron-curvature radiation as predicted by outer gap models. These GeV gamma-rays from unresolved millisecond pulsars probably contribute to the diffuse gamma-ray spectrum detected by EGRET which displays a break at a few GeV. We have used a Monte Carlo method to obtain simulated samples of millisecond pulsars in the Galactic Centre region covered by EGRET  (∼ 15)  according to the different period and magnetic field distributions from observed millisecond pulsars in the Galactic field and globular clusters, and superposed their synchrotron-curvature spectra to derive the total GeV flux. Our simulated results suggest that there probably exist about 6000 unresolved millisecond pulsars in the region of angular resolution of EGRET, the emissions of which could contribute significantly to the observed diffuse gamma-rays in the Galactic Centre.     

基于重心模型的环境污染和治理投资偏离分析

利用重心的概念和模型,采用2000-2009年各省工业废水、工业废气和工业固体废弃物的排放量和污染治理投资额等数据,计算出各自的重心和重心演变路径．从移动方向、移动距离和相互关系3个方面分析环境污染重心和治理投资重心各自的动态变化和空间演变轨迹,结果显示：2000-2009年,工业废水、废气和固体废弃物污染重心从移动方向来看总体向西部偏移,而且移动距离有快速西移的趋势,表明当前西部地区在环境污染方面有加重的趋势．另外,环境污染重心和投资治理重心之间存在偏离,例如,工业废水排放重心偏北,而工业废水治理投资重心偏南,并且与工业废水重心相比,工业废气和工业固体废弃物排放重心和治理投资重心偏离度要小．