Efficiency tests for estimating the gas and stellar population parameters in Type 2 objects

We investigated the efficiency of estimating characteristics of stellar populations (SP) and Active Galactic Nuclei (AGN) emission using ULySS code. To analyze simultaneously AGN and SP components in the integrated spectrum of Type 2 active galaxies, we modeled the featureless continuum (FC) and emission lines, and we used PEGASE.HR stellar population models provided by ULySS. In order to validate the method, we simulated over 7000 integrated spectra of Seyfert 2 galaxies. Spectra were generated using different characteristics of the featureless AGN continuum, signal-to-noise ratio (SNR), spectral ranges, properties of emission lines and single stellar population (SSP) model whose initial mass function (IMF) and abundance pattern is similar to the solar neighborhood. Simulated spectra were fitted with ULySS to evaluate the ability of the method to extract SP and AGN properties. We found that the analysis with ULySS can efficiently restore the characteristics of SP in spectra of Seyfert 2 AGNs, where signal-to-noise ratio is higher than 20, and where SP contributes with more than 10% to the total flux. Degeneracies between AGN and SP parameters increase with increasing the AGN continuum fraction, which points out the importance of simultaneous fitting of the FC and SP contributions.     

分布式通用航空服务站系统功能与组成研究

分布式通用航空服务站系统是针对通用航空领域建设的地面设施系统,除具备现有通用航空服务站的基本功能外,还具备飞行情报中心处理功能,能够将辖区范围内各服务站终端的数据分类接收、汇总和处理,形成空地一体化空中交通服务网络,为通航用户提供更全面、更可靠的信息服务,提高通用航空飞行安全保障水平。本文在分析国内外航空服务站功能的基础上,结合我国国情和通用航空发展情况,提出了分布式通用航空服务站系统的概念,详细说明了飞行情报中心功能特点,并与传统航空服务站进行了对比,对完善我国通用航空管理信息服务保障体系、促进低空空域发展具有一定的借鉴意义。     

通用航空产业发展途径探讨

通用航空由于应用范围广且对经济有较强的拉动作用,受到了各级政府部门的重视,国家的＂十二五＂规划已经将其列为国家的战略新兴产业。针对我国通用航空发展极度落后的现状,分析了制约通用航空产业发展的主要因素,包括空域管制、通用航空法律法规不健全、专业人才短缺以及航空保障设施落后等,探讨了通用航空产业的发展途径,提出了加强宣传、政府主导、专业人才培养等一些有价值的建议。     

Magnetogasdynamic shock wave generated by a moving piston in a rotational axisymmetric isothermal flow of perfect gas with variable density

The propagation of a strong cylindrical shock wave in an ideal gas with azimuthal magnetic field, and with or without axisymmetric rotational effects, is investigated. The shock wave is driven out by a piston moving with time according to power law. The ambient medium is assumed to have radial, axial and azimuthal component of fluid velocities. The fluid velocities, the initial density and the initial magnetic field of the ambient medium are assumed to be varying and obey power laws. Solutions are obtained, when the flow between the shock and the piston is isothermal. The gas is assumed to have infinite electrical conductivity and the angular velocity of the ambient medium is assumed to be decreasing as the distance from the axis increases. It is expected that such an angular velocity may occur in the atmospheres of rotating planets and stars. The shock wave moves with variable velocity and the total energy of the wave is non-constant. The effects of variation of the initial density and the Alfven-Mach number on the flow-field are obtained. A comparison is also made between rotating and non-rotating cases.     

GRB host galaxies: An unbiased sample

We describe the current status and recent results from our Swift/VLT legacy survey, a VLT Large Programme aimed at characterizing the host galaxies of a homogeneously selected sub-sample of Swift   GRBs. The immediate goals are to determine the host luminosity function, study the effects of reddening, determine the fraction of Lyα$\mathrm{Ly}\mathrm{\alpha }$ emitters in the hosts, and obtain redshifts for targets without a reported one. The main effort so far has been the definition of a very carefully selected sample, obeying strict and well-defined criteria: 68 targets in total. Among the preliminary results is a large optical detection rate, the lack of extremely red objects (only one possible case in the sample) and an update of the Swift   GRB redshift distribution with 〈z〉∼2.0$〈z〉\sim 2.0$.     

Pulsar radio emission

25 years after their discovery, pulsars still pose fundamental problems, in particular when the whole range of their periodsP is considered: 1.56 ms P0.09 s. This communication reviews my understanding of the pulsar magnetosphere, windzone, and (coherent) radio emission. New are details of the preferred magnetic structure, wind generation, and amplification of the emitted (pseudo) curvature radiation, the inferred brightness of which exceeds that of all other terrestrial and astrophysical sources by many orders of magnitude.     

美国通用航空产业发展的经验剖析及启示

美国是世界通用航空产业最为发达的国家,其发展得益于政府实施的产业政策和保障措施。与美国相比,我国通用航空产业发展仍处于起步阶段。伴随着中国经济结构转型升级,我国通用航空产业将迎来良好发展机遇。因此,应该借鉴美国发展通用航空产业的经验,在顶层设计上统筹规划,构筑和完善符合中国实际的法律与政策体系,出台相关具体措施,以推动我国通用航空产业健康较快发展。     

涡轴发动机通用仿真平台研究

采用部件法建立涡轴发动机通用模型的难点是:如何为发动机模型的各部件参数和特性数据块建立统一的输入接口;建立的稳态模型和动态模型均要在全包线范围内收敛;动态模型要求在任意高度和马赫数下均能满足实时性要求.文章利用Vc++编程语言建立了统一特性数据输入接口;综合使用多种方法使数学模型达到全包线范围内收敛和满足实时性要求的目的.     

Massive star distribution in external galaxies and starburst regions

Counts of hot and luminous stars in a number of associations in the Galaxy and Magellanic Clouds enable one to directly investigate the numbers and types of massive stars. There seems to be little, if any, dependence of the slope of the Intial Mass Function, or theM _upper on the initial composition of the stars. Indirect estimates of numbers of massive stars in various more distant environments are reviewed and discussed within a framework of acalibration of the methods using the stellar census of 30 Doradus. Very young starbursts, containing large numbers of massive stars, seem to be composed of smaller sub-units similar or somewhat larger than that object. These units might be newly born globular clusters.     

债转股问题初探

债转股作为经济体制改革的一个重要探索，已经成为当今法学界和经济学界讨论的主题。作为一个新事物的出现，债转股必然会遇到一系列来自不同方向的阻碍，本文就这些困惑进行论述，阐明了债转股面临的主要问题，并提出相应的解决方案和建议。国民经济体制改革需要大胆的探索和创新，债转股就是一个很好的范例，尽管其实施过程中难免遇到一些难题，但必将取得骄人的成果。