The Hybrid Nature of 0846＋51W1： a BL Lac Object with a Narrow Line Seyfert 1 Nucleus

We found a NLS1 nucleus in the extensively studied eruptive BL Lac object, 0846+51W1, out of a large sample of NLS1s compiled from the spectroscopic dataset of SDSS DR1. Its optical spectrum can be well decomposed into three components: a power law component from the relativistic jet, a stellar component from the host galaxy, and a component from a typical NLS1 nucleus. The emission line properties of 0846+51W1, FWHM     

我国交通设施沿线固沙措施与技术研究综述

流沙是我国沙漠化主要成因之一。本文简要回顾了我国北方沙漠及受沙漠化影响的干旱半干旱地区为保护交通线路而采取的固沙措施和技术,包括工程措施、化学措施和生物措施,主要介绍了这些措施和技术的类型及特点,以及近60年间(1950–2010年)其在不同地区不同交通线路中的应用,包括包兰线、塔里木沙漠公路和青藏铁路沿线的防风固沙。工程措施,如建挡风墙和铺设沙障,在沙漠交通线的防风固沙中非常有效。化学措施因成本高和对环境可能造成的污染风险而应用并不普遍。生物措施比工程和化学措施成本更高,但因其效果好且防护持续时间长而得到推崇。在一些地方,几种措施组合的固沙效果更好。工程措施对沙面的固定以及有条件的地方用地下水或河水灌溉有助于旱生植物的早期定植。本文最后指出了固沙措施和技术的局限性以及未来研究方向。本文对解决蒙古高原受沙漠和沙漠化影响的干旱和半干旱地区与"一带一路"倡议相关的基础设施建设的生态环境问题具有重要意义。     

A disturbed molecular disc in the Circinus galaxy

We have used the Swedish ESO Submillimeter Telescope to observe the molecular gas in the Circinus galaxy using the CO(1 → 0) transition as a tracer. The central region and major axis have been mapped and several other points were also observed. The gas in the galaxy is concentrated towards the nucleus, the peak being coincident with the radio/optical core. The inclination of the molecular galactic disc is more comparable to that of the radio continuum than to that of the large-scale H  i emission. Evidence for an anomalous spur structure pointing radially away from the galactic centre is presented, and may indicate a causal link between it and similar features seen in optical lines and radio continuum. Our data suggest the presence of a central molecular ring or disc with radius 300 ± 50 pc and a rotation velocity of about 200 km s⁻¹ (assuming i  = 73°). The dynamical mass of the nucleus is estimated to be no greater than 3.9 × 10⁹ M_⊙. Assuming that the distribution of gas varies smoothly in the outer regions, we calculate the mass of molecular gas in the galaxy to be at least M _mol = 1.1 × 10⁹ M_⊙, and the star-forming efficiency to be 11 ± 2 L_⊙ M_⊙⁻¹. These results imply that Circinus is undergoing a massive central starburst which may be, at least partially, responsible for its extended minor axis emission seen in several wavebands.     

GMRT observations of interstellar clouds in the 21cm line of atomic hydrogen

Nearby interstellar clouds with high (|ν|≥10km s⁻¹) random velocities although easily detected in NaI and CaII lines have hitherto not been detected (in emission or absorption) in the HI 21cm line. We describe here deep Giant Metrewave Radio Telescope (GMRT) HI absorption observations toward radio sources with small angular separation from bright O and B stars whose spectra reveal the presence of intervening high random velocity CaII absorbing clouds. In 5 out of the 14 directions searched we detect HI 21cm absorption features from these clouds. The mean optical depth of these detections is ∼0.09 and FWHM is ∼10km s⁻¹, consistent with absorption arising from CNM clouds.     

基于等高线隔断线确定DEM适宜分辨率的方法研究

分辨率是等高线数据插值生成格网DEM数据过程中需要考虑的一个重要参数,适宜的分辨率既能将等高线高程信息尽可能保留,又不会因插值造成数据冗余及误差。基于对格网DEM生成方式的理解,提出了等高线隔断线的相关概念,分析了基于地形图矢量化的等高线数据插值生成格网DEM数据,由不同长度等高线隔断线频率统计来确定格网适宜分辨率参考值的方法。同时,不同长度等高线隔断线的长度与其频率相乘得到标准长度,以及等高线隔断线中心点生成的密度分析图,均可在频率特征决定适宜分辨率参考值时起到一定的参考作用。通过样区实验验证,实现简便,可度量性强,与其他相关研究具有一致性,对确定适宜格网分辨率参考值具有一定的借鉴意义。     

基于地性线分级的DEM信息量计算方法研究

主要对基于DEM提取的地性线进行信息量的定量分析,探讨地性线的信息量与分辨率、地形单元的关系。这个过程中首先利用河网的自相似理论研究与当前DEM所代表的地貌详细程度相适宜的地性线提取的阈值区间,并讨论此阈值下地性线的分级,以此为基础通过以该分级为权重进行DEM地形信息量的计算。实践证明,这种顾及地性线等级的DEM信息量计算方法能较准确地反映地性线的分布规律和不同等级的要素造成的信息量度量差异。     

湖南白兔潭矿区荷田区段构造特征与找煤前景

煤炭是湖南省的主要能源,经过多年的勘探开发,暴露区和浅部的煤炭资源已基本采完,因此,在隐伏区寻找新的煤炭资源已成为当务之急。隐伏区找煤主要指“三下”(老地层下、构造下和红层下)找煤,而“老地层下和构造下”找煤主要是指利用推覆构造理论寻找新的煤炭资源。为了深化对区域构造和煤田构造发育规律的认识,为本区煤炭资源勘探和矿井生产地质保障提供新思路、开拓新领域,以当代构造地质理论为指导,结合已有资料,对白兔潭矿区荷田区段的煤田构造进行了研究,揭示了煤田的构造格局,提出了该区可能存在的两种构造模式,对该区找煤前景做出了科学评价,指出了可供进一步勘探的有利区段。     

重磁等值线与经纬网的分离及其矢量化

本文利用经纬网在局部范围的直线性直线的平均ｆｒｅｅｍａｎ链码等于其上任意一点的链码的这一特性,达到自动分离经纬网与等值线的目的,为实现等值线图的自动矢量化打下了基础。