Hard X-ray observations of Cygnus X-1 with the MISO telescope

The black hole candidate Cygnus X-1 was observed in the hard X ray - soft γ ray energy range by the MISO telescope on two different occasions: in September 1979 and May 1980. We have measured two hard X-ray states of the source: in 1979 the observed spectrum confirms the superlow state measured in the same period by the HEAO-3 satellite, while in 1980 the MISO X-ray data are consistent with the so called low state of Cygnus X-1. In both occasions, no γ -ray excess has been observed above 200 KeV.     

The role of ultraviolet imaging in studies of resolved and unresolved young stellar populations. M31 and M33

We discuss the relevance of UV data in the detection and characterization of hot massive stars and young stellar populations in galaxies. We show results from recent extensive surveys in M31 and M33 with Hubble Space Telescope (HST) multi-wavelength data including UV filters, which imaged several regions at a linear resolution (projected) of less than half a pc in these galaxies, and from GALEX far-UV and near-UV wide-field, low-resolution imaging of the entire galaxies. Both datasets allow us to study the hierarchical structure of star formation: the youngest stellar groups are the most compact, and are often arranged within broader, sparser structures. The derived recent star-formation rates are rather similar for the two galaxies, when scaled for the respective areas. We show how uncertainties in metallicity and type of selective extinction for the internal reddening may affect the results, and how an appropriate complement of UV filters could reduce such uncertainties, and significantly alleviate some parameter degeneracies.     

类X-47狭缝式进气道的流动特征与工作性能

对一种背部安装的狭缝式进气道进行了设计和仿真研究,获得了该类进气道的流动特征和工作特性.结果表明,由于存在剧烈的通道弯曲和宽度收缩,进气道的内部流动较为恶劣,边界层气流在通道的上方和下方两侧堆积,并在扩压器后段的上部出现了分离.当自由流马赫数为0.70、迎角为0.时,进气道出口截面的总压恢复系数为0.975,总压畸变指数则达0.484.另外,进气道前方的大鼓包未能起到有效排除前体边界层气流的效果,而正迎角下前体侧棱产生的前缘涡则能将前体边界层扫向机体的两侧,有效减少了进入内通道的低能气流,对出口截面下方两侧的低总压区起着抑制作用.本文的工作还为狭缝式进气道的改进设计提供了依据.     

航空发动机CCAR33-R2.75条款适航符合性验证方法研究

针对航空发动机适航取证的安全性需求,对航空发动机CCAR33-R2.75适航条款进行了解读与分析,明确了该条款的验证要求和方法.将功能危险分析法、故障树分析法和故障模式与影响分析法运用到该验证方法中,并提出了航空发动机CCAR33-R2.75条款适航符合性验证的流程.最后对某型航空发动机进行实例分析,验证了发动机不可控火情对CCAR33-R2.75条款的符合性.该安全性验证方法能够为航空发动机CCAR33-R2.75条款适航符合性验证提供支持.     

3J33C小孔镗削温度测量实验及有限元模拟

基于3J33C弹性合金小孔镗削温度测量实验及Advant Edge有限元温度仿真试验,验证了有限元模型及结果的可靠性,得到其不同镗削参数时基体最高温度的变化规律及温度范围。基于有限元仿真结果建立了3J33C小孔镗削的温度经验公式,结果表明,随着镗削转速、进给速度及径向切深的增大,镗削温度都呈现升高趋势,并且在这三个因素中镗削转速影响最大,进给速度影响次之,径向切深影响最小。     

高超音速技术发展概述

简述了美国高超音速飞行器计划的研制背景,介绍了乘波者飞行器的构型特点与热应力松弛设计考虑,初步探讨了高超音速验证飞行器的典型代表X-51A和HTV-2验证飞行失败的原因与遇到的技术困难。     

Cyg X-2 — An accreting neutron star

HAKUCHO observation of Cyg X-2 over 40 days did not show a correlation between the hardness ratio and the intensity predicted for dwarf X-ray sources. The energy spectrum in the range 0.3 – 20 keV was found to deviate from the thermal bremsstrahlung spectrum below 2 keV. The X-ray spectrum can be accounted for in terms of the comptonization of blackbody radiation emitted from teh neutron star surface and the accretion disk.     

Cosmic background radiation from pregalactic objects

X-ray astronomy satellite TENMA observed that the X-ray pulsation of Vela X-1 suddenly disappeared for tens of minutes. This phenomenon may be interpreted in terms of the eclipse by a planet of HD77581, the optical companion of Vela X-1.