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201.
R.N. Manchester 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2709-2715
Recent pulsar surveys, especially those using the multibeam receiver on the Parkes radio telescope, have more than doubled the number of known pulsars, bringing the current total to about 1720. Of these, 171 have millisecond periods, 126 are members of binary systems and 99 are associated with globular clusters. Binary pulsars may be divided into several distinct groups depending on their observed properties such as pulsar period and age, binary period, eccentricity and companion mass. These groups all have different evolutionary histories. Correlations between the various properties are discussed using the increased samples now available. The Parkes Pulsar Timing Array is a project which has the goal of using timing observations of millisecond pulsars to make a direct detection of gravitational waves. The parameters and present status of the project are briefly discussed. 相似文献
202.
N.A. Webb D. Barret B. Gendre 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2930-2933
Using the new generation of X-ray observatories, we are now beginning to identify populations of close binaries in globular clusters, previously elusive in the optical domain because of the high stellar density. These binaries are thought to be, at least in part, responsible for delaying the inevitable core collapse of globular clusters and their identification is therefore essential in understanding the evolution of globular clusters, as well as being valuable in the study of the binaries themselves. Here, we present observations made with XMM-Newton of six globular clusters, in which we have identified neutron star low mass X-ray binaries and their descendants (millisecond pulsars), cataclysmic variables and other types of binaries. We discuss not only the characteristics of these binaries, but also their formation and evolution in globular clusters and their use in tracing the dynamical history of these clusters. 相似文献
203.
等维灰数递补动态预测在机场客运量预测中的应用 总被引:1,自引:0,他引:1
基于灰色系统等维灰数递补动态预测和残差GM(1,1)修正模型,对其应用的可行性进行了有益的探讨,并结合实例,对首都国际机场中短期客运量进行了预测。通过调整原始样本中的变异数据,得到比较理想的预测结果.经检验预测结果是可信的。该研究为机场客运量预测提供了一种方法,可供借鉴。 相似文献
204.
J. S. Kaastra F. B. S. Paerels F. Durret S. Schindler P. Richter 《Space Science Reviews》2008,134(1-4):155-190
We discuss the different physical processes that are important to understand the thermal X-ray emission and absorption spectra
of the diffuse gas in clusters of galaxies and the warm-hot intergalactic medium. The ionisation balance, line and continuum
emission and absorption properties are reviewed and several practical examples are given that illustrate the most important
diagnostic features in the X-ray spectra. 相似文献
205.
雷达对抗仿真通用系统架构研究 总被引:1,自引:0,他引:1
分析了在雷达对抗仿真系统研制过程中,建立通用的系统架构带来的好处,并从仿真系统体系结构和功能设计两个方面,提出了实现通用系统架构的基本技术思路和方法。 相似文献
206.
基于PC/104总线的飞机电源产品综合测试系统 总被引:1,自引:0,他引:1
详细介绍了一套基于PC/104总线和虚拟仪器技术的飞机电源产品综合测试系统的功能和软硬件实现原理。阐述了测试系统的设计原理,最后结合整个系统设计介绍了在LabVIEW环境下测试系统软件的设计和实现。 相似文献
207.
针对纳米到皮米量级星间激光测距,在地心非旋转坐标系(GCRS)下,考虑卫星轨道摄动引起的广义相对论效应,建立了星间单向以及双向星间激光相位比对模型.通过仿真研究了地球主引力场范围内轨道摄动引起的广义相对论效应对星间激光相位比对误差的影响,并通过星间激光相位比对误差计算星间激光测距误差.不同轨道高度的卫星仿真结果表明,对... 相似文献
208.
气动发动机多参数多目标寻优方法 总被引:1,自引:0,他引:1
气动发动机设计需要考虑多个参数间的耦合对性能优化的影响,且对理想功率、工作效率等多个性能指标难以建立客观的综合评价函数.为此以发动机进气压力和进排气机构部分控制参数为设计变量进行正交设计,利用灰色关联度分析法计算贴合期望指标组合的最优参数组合,并结合参数指标趋势图,依据计算结果对参数区间进行调整,通过有限次循环得到最优设计参数.经测试该算法快速有效,且设计参数与性能指标数量可扩展,对气动发动机的样机设计和实验具有重要的理论和工程意义. 相似文献
209.
M.T. Menna A. Papitto L. Burderi T. Di Salvo F. DAntona N.R. Robba 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2704-2706
We analyze the three outbursts of the X-ray millisecond pulsar SAX J1808.4-3658 that occurred in 1998, 2000, and 2002 observed with RXTE. With a technique based on epoch folding search we find an unique orbital solution valid over the five years of high temporal resolution data available. We revise the estimate of the orbital period, Porb = 7249.1569(1) s and of its error, which we decrease by one order of magnitude. We also give the first constraint on the orbital period derivative, . We find that in 2002 the pulse profile shape is clearly asymmetric, showing a secondary peak at about 145° from the main pulse, which is different from the sinusoidal shape reported at the beginning of the 1998 outburst. 相似文献
210.