Emission-line properties of Seyfert 2 nuclei

This is the third paper of a series devoted to the study of the global properties of Joguet's sample of 79 nearby galaxies observable from the southern hemisphere, of which 65 are Seyfert 2 galaxies. We use the population synthesis models of Paper II to derive 'pure' emission-line spectra for the Seyfert 2 galaxies in the sample, and thus explore the statistical properties of the nuclear nebular components and their relation to the stellar populations. We find that the emission-line clouds suffer substantially more extinction than the starlight, and we confirm the correlations between stellar and nebular velocity dispersions and between emission-line luminosity and velocity dispersions, although with substantial scatter. Nuclear luminosities correlate with stellar velocity dispersions, but Seyferts with conspicuous star-forming activity deviate systematically towards higher luminosities. Removing the contribution of young stars to the optical continuum produces a tighter and steeper relation,   L ∝σ⁴_★  , consistent with the Faber–Jackson law.
Emission-line ratios indicative of the gas excitation such as [O  iii ]/Hβ and [O  iii ]/[O  ii ] are statistically smaller for Seyferts with significant star formation, implying that ionization by massive stars is responsible for a substantial and sometimes even a dominant fraction of the Hβ and [O  ii ] fluxes. We use our models to constrain the maximum fraction of the ionizing power that can be generated by a hidden active galactic nucleus (AGN). We correlate this fraction with classical indicators of AGN photoionization (i.e. X-ray luminosity and nebular excitation), but find no significant correlations. Thus, while there is a strong contribution of starbursts to the excitation of the nuclear nebular emission in low-luminosity Seyferts, the contribution of the hidden AGN remains elusive even in hard X-rays.     

抽真空引起周围土体竖向变形的有限元分析

真空预压法加固深厚超软土地基时,一方面使地基土体产生侧向收缩变形,有利于地基的稳定;但另一方面向真空预压区的侧向变形对周围房屋、地下管线、道路等建筑物也产生不利影响,甚至会出现管道断裂、围墙倒塌、路堤被毁等严重工程事故。结合真空预压加固软基工程中出现的对周围环境影响的问题,进行了考虑土体拉裂影响的有限元分析,研究抽真空过程及加固区外不同距离、不同土体深度沉降的变化规律。研究结果表明,采用Biot固结理论、考虑土体拉裂的有限元计算结果与现场加固区外土体沉降及影响区范围的实测结果基本一致。     

Chemical abundances and ionizing clusters of H ii regions in the LINER galaxy NGC 4258

We present long-slit observations in the optical and near-infrared of eight H  ii regions in the spiral galaxy NGC 4258. Six of the observed regions are located in the south-east inner spiral arms, and the other two are isolated in the northern outer arms. A detailed analysis of the physical conditions of the gas has been performed. For two of the regions, an electron temperature has been derived from the [S  iii ] λ 6312 line. For the rest, an empirical calibration based on the red and near-infrared sulphur lines has been used. The oxygen abundances derived by both methods are found to be significantly lower (by a factor of 2) than previously derived by using empirical calibrations based on the optical oxygen lines.
In the brightest region, 74C, the observation of a prominent feature caused by Wolf–Rayet (WR) stars provides an excellent constraint over some properties of the ionizing clusters. In the light of the current evolutionary synthesis models, no consistent solution is found to explain at the same time both the WR feature characteristics and the emission-line spectrum of this region. In principle, the presence of WR stars could lead to large temperature fluctuations and also to a hardening of the ionizing radiation. None of these effects is found in region 74C, for which the electron temperatures found from the [S  iii ] λ 6312 line and the Paschen discontinuity at 8200 Å are equal within the errors, and the effective temperature of the ionizing radiation is estimated at around 35 300 K.
Both more observations of confirmed high-metallicity regions and a finer metallicity grid for the evolutionary synthesis models are needed in order to understand the ionizing populations of H  ii regions.     

Stellar indices and kinematics in Seyfert 1 nuclei

We present spectra of six type 1 and two type 2 Seyfert galaxies, a starburst galaxy and a compact narrow-line radio galaxy, taken in two spectral ranges centred around the near-infrared Ca  ii triplet (∼8600 Å), and the Mgb stellar feature at 5180 Å. We measured the equivalent widths (EWs) of these features and the Fe₅₂ and Fe₅₃ spectral indices.
We found that the strength of the infrared Ca  ii triplet (CaT) in type 1 Seyfert galaxies with prominent central point sources is larger than what would be expected from the observed strength of the blue indices. This could be explained by the presence of red supergiants in the nuclei of Seyfert 1 galaxies. On the other hand, the blue indices of these galaxies could also be diluted by the strong Fe  ii multiplets that can be seen in their spectra.
We have also measured the stellar‐ and gas-velocity dispersions of the galaxies in the sample. The stellar velocity dispersions were measured using both the Mgb and CaT stellar features. The velocity dispersion of the gas in the narrow-line region (NLR) was measured using the strong emission lines [O  iii ] λλ 5007, 4959 and [S  iii ] λ 9069. We compare the gas- and star-velocity dispersions and find that the magnitudes of both are correlated in Seyfert galaxies.
Most of the Seyfert 1 galaxies that we observe have stellar‐velocity dispersions somewhat greater than that of the gas in the NLR.     

河网自动综合中Delaunay三角的应用

在地图数据处理和GIS分析应用中,河网自动综合是制图综合的一个重要组成部分,其中涉及到从双线河向单线河转化的过程及河间距的研究。本文利用Delaunay三角网中的三角形的边连接具有的空间邻近性特点,介绍了用Delaunay三角网结构的骨架线来提取双线河流中轴线及研究河间距量算的方法。     

国土资源调查数据地图综合狭长图斑的中剖分处理

国土资源调查获得的土地利用图在服务不同层次、不同级别国土规划管理应用中,面临着多级数据库建设与地图综合缩编的任务需求.土地利用图中狭长图斑的中轴化是其中不可缺少的关键操作之一.针对土地利用数据全覆盖、无重叠、无缝隙及语义上多层次的特点,本文提出一种密集覆盖多边形数据的中轴化处理与拓扑关系维护的方法,用“剖分”与“归并”的思想模拟邻域多边形的扩张过程.本文算法实现建立在Delaunay三角网数据结构上,兼顾了语义相似关系的影响,经第三次国土资源调查成果的检验,本文所述中轴化及拓扑维护方法能够满足土地利用图综合实际生产的需要.     

一种循序渐进的无人机航测实践教学模式

以有效培养学生实践能力为目标,提出了一种循序渐进的无人机航测实践教学模式,分为基本能力实训和强化能力实训.基本能力的外业实训通过无人机地面站设置2D航线以获取垂直影像,内业实训利用数字摄影测量网格系统(Digital Photogrammetric Grid,DPGrid)软件生产数字高程模型(Digital Elevation Model,DEM)、数字正射影像(Digital Orthophoto Map,DOM)、数字线划地图(Digital Line Graphic,DLG),Pix4Dmapper软件生产数字地表模型(Digital Surface Model,DSM)、DOM,DPGrid软件分模块按步骤执行且人机交互多,更适合学生基本能力的实践教学;强化能力的外业实训通过无人机地面站设置3D航线以获取倾斜影像,内业实训通过Agisoft Metashape和ContextCapture软件进行倾斜影像处理,生产3D模型,ContextCapture软件的三维重建效果好,Agisoft Metashape软件的分模块按步骤执行过程详细,更适合学生强化能力的实践教学.     

鄂尔多斯东北部中侏罗世孢粉化石及古气候意义

鄂尔多斯盆地东北部内蒙古伊金霍洛旗乌兰木伦地区是我国重要的能源矿产地,含煤岩系赋存在侏罗系延安组中,延安组岩石组合以灰白色砂岩、灰色粉砂岩、灰色泥岩为主,夹多层煤层;延安组上覆直罗组以灰色、灰绿色砂岩、灰色粉砂岩、紫红色泥岩为主。通过对乌兰木伦地区武家塔露天煤矿剖面延安组和直罗组孢粉化石分析,在延安组中识别出Cyathidites-Lycopodiumsporites-Neoraistrickia-Cycadopites孢粉组合带,以桫椤科、石松科孢子繁盛,紫萁科孢子和单沟/原始沟类、松柏类两气囊花粉发育,卷柏科孢子及柏科花粉较常见为主要特征,时代为中侏罗世早期(阿林期—巴柔期)。根据延安组孢粉母体植物的生态环境分析,本区在这一沉积时期的气候属于温暖湿润的亚热带—温带型气候。直罗组孢粉化石较少,主要见Cyathidites minor,Osmundacidites parvus,Concentrisporites fragilis,Cycadopites spp.等。综合地层岩性、孢粉组合及古植被分析,延安组到直罗组沉积时期总体上呈现从温暖湿润的亚热带—温带型向半干旱—干旱炎热型的气候...     

基于新型LE水平跳点网格的阴阳网格平流方案设计

为了模拟球面平流传输过程,本文基于球面阴阳重叠网格设计了一种两时间层半拉格朗日平流方案.该方案在球面坐标下采用新型的LE水平跳点网格,同时针对阴阳网格重叠区,采用了不同插值方法进行比较分析,且进行了相关的理想数值试验对方案设计效果进行评估.数值试验表明方案设计是成功的,阴阳网格重叠区平流对插值方案比较敏感;半拉格朗日方案能较好地模拟球面刚体平流和变形涡旋的结构、位置及演变过程,并具有较好的数值稳定性和较高的数值精度.     

云南哀牢山东侧一次突发性暴雨过程诊断分析

利用加密自动站资料、NCEP每6 h再分析资料和FY-2C红外TBB等资料,对2012年6月15日发生在哀牢山东侧突发性暴雨进行诊断分析。结果表明:700hPa切变线移到哀牢山后受滇缅脊和地形阻挡形成与山脉同向的切变线.地面冷锋移到哀山东侧后形成静止锋,受不断南下冷空气补充.形成冷空气下沉,暖湿气流上升,出现强烈的上升运动。切变线附近辐合云带内形成的中尺度对流云团在高空西北气流引导下产生的"列车效应"导致了突发性暴雨发生。来自东海和孟加拉湾水汽在切变线附近交汇,受切变线两侧风向辐合产生强烈的水汽辐合,并在哀牢山附近形成深厚的水汽辐合层,是本次突发性暴雨天气的主要水汽特征。逐小时地面自动站海平面气压场和对流有效位能在哀牢山沿线突发性暴雨发生前有明显变化,强降水主要发生在地面中尺度暖低压附近和对流有效位能高值区,此分析对此类短时强降水预报和预警具有一定指示意义。