Broad-band spectral properties of accreting X-ray binary pulsars

Broad-band spectra of accreting X-ray binary pulsars can be fitted by a phenomenological model composed of a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently, a qualitative picture able to explain the overall broad-band spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review of these recent theoretical developments, I will present a case study of how different modeling of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1.     

Near infrared studies of the massive X-ray binary 2S 0114+65

We present near-infrared spectroscopy of the massive X-ray binary 2S 0114+650. These observations covering the spectral range 1.08–2.35 μm span the region where Paschen and Brackett series recombination lines of hydrogen are expected to be seen, namely, Paβ , Brγ and Br 10–17 lines. The absence of any of these lines in emission supports earlier inferences that the optical component in 2S 0114+650 is unlikely to be a Be star but rather a B type supergiant. Near-IR photometry gives J = 8.78, H = 8.53 and K = 7.96; these values show marginal variations from earlier reported measurements.     

单兵自主导航技术发展综述

在卫星受限情况下的单兵自主导航技术是近年来研究的热点。首先介绍了单兵自主导航技术的发展概况,然后重点分析了基于MIMU的单兵惯性导航技术的主要原理和方法,之后针对纯惯性导航存在的问题,介绍了地磁、场景、视觉等常用的单兵辅助导航方法,并阐述了单兵协同导航技术。最后,简要介绍了单兵自主导航技术的未来发展趋势。     

Near-infrared study of open clusters Teutsch 10 and Teutsch 25

The astrophysical parameters have been estimated for two unstudied open star clusters Teutsch 10 and Teutsch 25 using the Two Micron All Sky Survey ($2\mathit{MASS}$) database. Radius is estimated as 4.5 arcmin for both clusters using radial density profiles. We have estimated proper motion values in both RA and DEC directions as $2.28\pm 0.3$ and $-0.38\pm 0.11$?mas?yr^?1 for Teutsch 10 and $0.48\pm 0.3$ and $3.35\pm 0.16$?mas?yr^?1 for Teutsch 25 using $\mathit{PPMXL}$¹ catalog. By estimating the stellar membership probabilities, we have identified 30 and 28 most likely members for Teutsch 10 and Teutsch 25 respectively. We have estimated the reddening as $E(B-V)=0.96\pm 0.3$?mag for Teutsch 10 and $0.58\pm 0.2$?mag for Teutsch 25, while the corresponding distances are $2.4\pm 0.2$ and $1.9\pm 0.1$?kpc. Ages of $70\pm 10$?Myr for Teutsch 10 and $900\pm 100$?Myr for Teutsch 25 are estimated using the theoretical isochrones of metallicity Z?=?0.019. The mass function slopes are derived as $1.23\pm 0.30$ and $1.09\pm 0.35$ for Teutsch 10 and Teutsch 25 respectively. Estimated mass function slope for both the clusters are close to the Salpeter value ($x=1.35$) within the errors. Estimated values of dynamical relaxation time are found to be less than cluster’s age for these objects. This concludes that both objects are dynamically relaxed. The possible reason for relaxation may be due to dynamical evolution or imprint of star formation or both.     

单管火焰筒内燃烧过程的反应动力学数值模拟

为了建立航空煤油替代燃料的反应机理,并对航空发动机燃烧过程进行详细反应动力学研究,选用正癸烷作为航空煤油的替代燃料,建立了该替代燃料的化学反应详细机理与简化机理。分别采用详细机理与简化机理对正癸烷在激波管中的着火过程、在预混燃烧炉内的燃烧过程进行了数值计算,并与实验结果进行了对比分析。同时,耦合该简化机理与CFD计算软件Fluent,对某单管火焰筒内燃烧过程、排放物及活性中间组分的生成规律进行了详细分析,并与采用C12H23为燃料的单步总包反应机理的计算结果进行了对比分析。结果表明,采用简化机理计算得到的着火延迟时间、反应物与各主要生成物摩尔分数的整体变化趋势与实验数据吻合较好;与采用C12H23为燃料的单步反应机理相比,采用正癸烷为替代燃料的简化反应机理能更好地对单管火焰筒的燃烧与排放特性进行详细的动力学分析。     

S5 0716+714: GeV variability study

The GeV observations by Fermi-LAT give us the opportunity to characterize the high-energy emission (100 MeV–300 GeV) variability properties of the BL Lac object S5 0716+714. In this study, we performed flux and spectral analysis of more than 3 year long (August 2008 to April 2012) Fermi-LAT data of the source. During this period, the source exhibits two different modes of flux variability with characteristic timescales of ∼75 and ∼140 days, respectively. We also notice that the flux variations are characterized by a weak spectral hardening. The GeV spectrum of the source shows a clear deviation from a simple power law, and is better explained by a broken power law. Similar to other bright Fermi blazars, the break energy does not vary with the source flux during the different activity states. We discuss several possible scenarios to explain the observed spectral break.     

一种基于移动辅助节点的单兵导航系统协同初始化算法

惯性导航系统凭借其自主性强、隐蔽性好、可靠性高的优势,在单兵作战、反恐救援中发挥越来越重要的作用。针对单兵惯性导航系统精度较低,在长期工作后精度下降严重,需要重新初始化的问题,以单兵与无人平台的协同作业为背景,提出了一种基于移动式辅助节点的单兵导航系统协同快速初始化方法。该方法以目标节点的角增量、位移增量信息与测距信息作为输入,采用粒子滤波技术对单兵导航系统的位置和航向进行协同估计。试验表明,该算法最少仅需1个辅助节点即可实现较好的单兵惯导系统位置和航向初始化。     

个人养老保险问题的思考

建立有中国特色的社会保障体系,是社会主义市场经济体制的重要组成部分。完善社会养老保险,提倡个人参加储蓄养老保险和医疗保险,是加快养老保险体制改革的步伐,使全体人民安居乐业,共享和谐的重要举措。     

单兵导航多传感器信息融合自适应滤波算法

基于足绑式INS的单兵导航系统,通过将惯性导航系统、人体运动学约束、磁强计等多传感器信息进行融合得到准确的单兵导航信息。对于匀速步行时的单兵导航,可采用普通Kalman滤波算法进行多传感器信息融合,但不能满足跑步等激烈运动模式下单兵导航需求。提出衰减记忆新息自适应Kalman滤波算法,可满足多步态模式下的单兵导航多源信息融合的需求,实验结果验证了算法的有效性。     

论个人所得税存在的问题及对策

个人所得税存在实行分项课征制 ,易使纳税人化整为零 ,逃避税收 ;征税范围过窄 ,调节力度有限 ;免征额过低 ,易使富人税变成穷人税 ;纳税申报以个人为准 ,未考虑家庭人口问题 ,有失公平 ;以及征管手段落后等问题 ,进而提出进一步完善现行个人所得税的对策 ,采用总额和分项课征制 ;扩大征税范围 ,严格控制减免税 ;合理确定扣除项目和扣除标准 ;提高免征额 ;加强个税征管力度等措施。