On kinematics of gas clouds in the broad-line region of active galactic nuclei and quasars

The kinematics of gas clouds in broad-line region of active galactic nuclei and quasars is considered. The motion of the clouds is governed by three forces — gravitational influence from the central supermassive body, radiational pressure from the continuum radiation, and resistance of the intercloud medium. Clouds moves radial but only outward motion gives a velocity field, which is in accordance with the observational data. The profiles of the permited lines are obtained in some simplify assumptions for the emissive capacity of the gas in clouds, and are in good agreement with the observational data. In the framework of the model under consideration there is a possibility to estimate some physical parameters of the nuclei such as mass of the central body and density of the intercloud medium.     

机械加工切削用量的优化

本文探讨了机械加工中,切削用量优化目标函数,优化数学模型,优化方法步骤。以期用该模式取代凭经验选定切削用量的方法,从而提高经济效益。     

浅谈施工企业降低工程成本的有效控制

在目前我国建筑市场竞争激烈的背景下,对于一个建筑企业而言,取得项目施工权固然重要,但合理控制并降低施工成本,在保证施工质量前提下取得相应利润回报更为关键,应从施工前、施工过程中、竣工后三个环节加以有效控制。     

Pro／ENGINEER在模具设计中的使用技巧

分析了Pro／ENGINEER进行模具设计的使用技巧，阐明了并行工程技术与Pro／ENGINEER软件相结合的重要性。     

社会转型时期市民心态特征及相应对策

改革触及了经济领域和上层建筑，并使之发生着深刻的变化，且调整了人们的社会关系、利益关系，从而造成了社会心态的多样性。本文通过对大量调查资料的研究分析，真实详细地描述了社会转型阶段人们（以北京、上海、沙市为例）各种心态的现状，及由此产生的一系列社会问题。通过深入细致地剖析，分析总结其产生的原因及正负效应，从而提出对各种心态应采取的相应措施、方法。     

机床实体模型复模态空间动位移显示技术的研究

介绍了用实体模型在复模态空间显示机床整机动位移的原理和方法。并在VC++6.0开发平台上用OpenGL语言开发了相应软件。解决了以往同类软件动画效果不能真实地表现实际机床整机的动态位移情况的难题。     

飞机带外挂对称结构振型局部化的参数影响

本文在文〔１〕研究的基础上，详细分析了飞机左右对称子结构间的耦合度以及外挂联接刚度失调量的大小等因素对振型局部化程度的影响。通过具体的数据揭示了各参数对局部化程序的影响规律。     

热力学中最小熵增原理在流体力学中的应用

本文运用非平衡态热力学中最小熵增原理,分析了层流和湍流流动在接近热力学平衡定态时的特性。特别是在湍流流动中,舍弃了以往一些经验性的假设,指出流动处于局部机械平衡时可由最小熵增原理导出速度和温度分布。反之亦揭示了充分发展的湍流遵循最小熵增原理的这一机理。     

航行情报服务(AIS)及其属性初探

本篇首次运用情报的广义属性从理论上分析和概括了航行情报的定义、宗旨和有关性质,并给出了航行情报服务的流程图和交流图。对促进和加强这一学科的教学研究有一定的参考意义。     

Very high energy gamma-ray sources

A brief review of very high energy gamma-ray astronomy achievements is presented. The results of observations of the Crab nebula, the Cygnus X-3, Vela pulsar, radiogalaxy Centaurus A and 2CG 195+4 show that all these objects are the sources of very high energy gamma-quanta. The most powerfull source is Cygnus X-3. Its gamma-ray luminosity is no less than 3·10³⁷ erg.s⁻¹. The upper limit of quanta energy is no less than 10¹⁶eV. All sources are variable in different time scales, from milliseconds up to years. The nature of all these sources is not known yet, but known ones are pulsars.