Chemical evolution of circumstellar matter around young stellar objects

Recent observational studies of the chemical composition of circumstellar matter around both high- and low-mass young stellar objects are reviewed. The molecular abundances are found to be a strong function of evolutionary state, but not of system mass or luminosity. The data are discussed with reference to recent theoretical models.     

X选BL Lac天体的某些性质

本文给出了包含５６个Ｘ选择的ＢＬＬａｃ天体（ＸＢＬｓ）的完备样品，得到了一些相互关系并讨论了ＸＢＬｓ的一些性质。     

Gamma-ray Emission from the γ-ray-loud BL Lac Objects

1 INTaoDUCTIONMany blazar-boe active galedes have recelltly been detected in MeVGeV 7-ray energyrange by detectors on board the Compton Ganuna-Ray Obsewtory (Von Mootigny et al. 1995;Hartman et al. 1999). More recently, TeV ends8ion is obsemd in some object8, such as Mrk421 (z = 0.031, Punch et al. l992), Mrk 501 (z = 0.034, Qbo et al. 1996), 1ES 2344 514(z == 0.044, Catanese et al. 1998), PKS 2155304 (z = 0.117, Chadwick et al. 1999), and1ES 1959 650 (z = 0.048, NisWa 1999). Th…     

冀豫环流动磁测异常与中等地震关系研究

利用冀豫环流动地磁观测资料,绘制单点时序变化曲线,采用常规差值法,计算相邻两期的差值,绘制整个测区的平面等值线;分析研究1998年以来测区周围发生的中等地震与流动地磁数据变化的关系。结果显示,冀豫环流磁异常与邻区的中等地震有一定的对应关系,震前有两个或多个测点同时出现异常,而且异常特征表现为上升正异常。     

云南测震台网的大震应对方案改进——汶川地震监测启示

5·12汶川大地震后,根据现行测震台网运行中暴露出的一些问题,本文就震后流动观测台网的组建,大震限幅及测震台网中心备份3方面提出了改进方案,以保证云南省数字化地震观测台网在大地震来临时仍然能够正常运行。     

车载视频图像序列卡尔曼滤波及其移动量测应用

提出了一种基于特征对应和扩展卡尔曼滤波的运动与结构重建方法,对运动与结构重建在车载视频移动量测中的应用问题进行了分析研究,结合立体视频量测技术,在移动量测系统中对该方法进行了检验。结果表明,文中方法正确可行,精度较高,抗噪性能好,具有很好的移动量测应用价值。     

Optical intra-day variability timescales and black hole mass of the blazars

In this paper, we have used optical intra-day variability archive data to calculate the central black hole masses and Eddington luminosities for nine blazars: 3C 66A, AO 0235+164, S5 0716+714, PKS 0735+178, OJ 287, 1215+303, 1216−010, 1308+326, PKS 1510−089, Mrk 501 and BL Lac using intra-day variability timescales and periodicity (if present). The calculated central black hole mass of these nine blazars using intra-day variability timescales are found to be in the range of 1.22-25.30 × 10⁷ M_⊙ and corresponding Eddington luminosity in the range of 1.58-32.88 × 10⁴⁵ erg s⁻¹. The black hole mass and Eddington luminosity are in the range of 0.32-31.23 × 10⁸ M_⊙ and 1.23-31.20 × 10⁴⁶ erg s⁻¹, respectively when optical Doppler factor is taken into account. The comparison show, our estimated values of black hole mass are consistent with earlier reported values. Periodicity were present in two blazars OJ 287 and 1216−010 which give the central black hole mass of these blazars in the range of 1.32-14.6 × 10⁷ M_⊙ and corresponding Eddington luminosity in the range of 1.60-19.0 × 10⁴⁵ erg s⁻¹, respectively.     

基于移动车载测量模式下的测绘一体化应用

介绍了一种以机动车为设备搭载和作业平台,搭载测绘保障通用设备、卫星导航、数据传输和测量数据处理系统,实现数据采集、传输、处理、检核、发布与服务的测量内外业一体化应用,改变了传统测绘技术手段单一、分散及内外业相互脱节的作业模式。     

Design and implementation of framework of mobile GIS based on phone terminal for environmental monitoring

This paper proposes a method for constructing an extensive wireless GIS network by utilizing Java cellular phone as GIS terminal for environmental monitoring through dynamic location disaster-emergency notification management of spatial databases. An experimental case study is demonstrated to show its potential in the application field.     

Particle-acceleration time-scales in TeV blazar flares

Observations of minute-scale flares in TeV Blazars place constraints on particle-acceleration mechanisms in those objects. The implications for a variety of radiation mechanisms have been addressed in the literature; in this paper, we compare four different acceleration mechanisms: diffusive shock acceleration, second-order Fermi, shear acceleration and the converter mechanism. When the acceleration time-scales and radiative losses are taken into account, we can exclude shear acceleration and the neutron-based converted mechanism as possible acceleration processes in these systems. The first-order Fermi process and the converter mechanism working via synchrotron self-Compton (SSC) photons are still practically instantaneous, however, provided sufficient turbulence is generated on the time-scale of seconds. We propose stochastic acceleration as a promising candidate for the energy-dependent time delays in recent gamma-ray flares of Markarian 501.