IU Cancri:a solar-type contact binary with mass transfer     

Hui-Yu Yuan  Hai-Feng Dai  Yuan-Gui Yang 《天文和天体物理学研究(英文版)》2019,(6):89-96

We present new CCD photometry of the solar-type contact binary IU Cnc, which was observed from November 2017 to March 2018 with three small telescopes in China. BV light curves imply that IU Cnc is a W-type contact binary with total eclipses. The photometric solution indicates that the mass ratio and fill-out factor are q = 4.104 ± 0.004 and f = 30.2%± 0.3%, respectively. From all available light minimum times, the orbital period may increase at a rate of dP/dt =+6.93(4)× 10^-7 d yr^-1, which may result from mass transfer from the secondary component to the primary one. With mass transferring,IU Cnc may evolve from a contact configuration into a semi-detached configuration.  相似文献   

ALMA observations of the circumstellar envelope around EP Aqr     

Pham Thi Tuyet Nhung  Do Thi Hoai  Pham Tuan-Anh  Thibaut Le Bertre  Pierre Darriulat  Pham Ngoc Diep  Nguyen Thi Phuong  Nguyen Thi Thao  Jan Martin Winters 《天文和天体物理学研究(英文版)》2019,(3):97-110

Atacama Large Millimetre/sub-millimetre Array(ALMA) observations of CO(1–0) and CO(2–1) emissions from the circumstellar envelope of the asymptotic giant branch(AGB) star EP Aqr have been made with four times better spatial resolution than previously available. They are analysed with emphasis on the de-projection in space of the effective emissivity and flux of matter using as input a prescribed configuration of the velocity field, assumed to be radial. The data are found to display an intrinsic axisymmetry with respect to an axis making a small angle with respect to the line of sight. A broad range of wind configurations, from prolate(bipolar) to oblate(equatorial) has been studied and found to be accompanied by significant equatorial emission. Qualitatively, the effective emissivity is enhanced near the equator to produce the central narrow component observed in the Doppler velocity spectra and its dependence on star latitude generally follows that of the wind velocity with the exception of an omni-present depression near the poles. In particular, large equatorial expansion velocities produce a flared disc or a ring of effective emissivity and mass loss. The effect on the determination of the orientation of the star axis of radial velocity gradients, and possibly competing rotation and expansion in the equatorial disc, is discussed. In general,the flux of matter is found to reach a broad maximum at distances of the order of 500 AU from the star.Arguments are given that may be used to favour one wind velocity distribution over another. As a result of the improved quality of the data, a deeper understanding of the constraints imposed on morphology and kinematics has been obtained.  相似文献   

New photometric investigation of the low-mass-ratio contact binary star V1853 Orionis     

Jia-Jia He  Sheng-Bang Qian  Boonrucksar Soonthornthum  Amornrat Aungwerojwit  Niang-Ping Liu  Thawicharat Sarotsakulchai 《天文和天体物理学研究(英文版)》2019,(4):77-88

Four-color charge-coupled device(CCD) light curves in the B, V, Rc and I c bands of the totaleclipsing binary system V1853 Orionis(V1853 Ori) are presented. By comparing our light curves with those published by previous investigators, it is determined that the O'Connell effect on the light curves has disappeared. By analyzing those multi-color light curves with the Wilson-Devinney code(W-D code),it is discovered that V1853 Ori is an A-type intermediate-contact binary with a degree of contact factor of f = 33.3%(3.7%) and a mass ratio of q = 0.1896(0.0013). Combining our 10 newly determined times of light minima together with others published in the literature, the period changes of the system are investigated. We found that the general trend of the observed minus calculated(O-C) curve shows a downward parabolic variation that corresponds to a long-term decrease in the orbital period with a rate of d P/dt =-1.96(0.46)×10^-7 d yr^-1. The long-term period decrease could be explained by mass transfer from the more-massive component to the less-massive one. By combining our photometric solutions with data from Gaia DR_2, absolute parameters were derived as M_1 = 1.20 M⊙, M_2 = 0.23 M⊙, R_1 = 1.36 R⊙and R_2 = 0.66 R⊙. The long-term period decrease and intermediate-contact configuration suggest that V1853 Ori will evolve into a high fill-out overcontact binary.  相似文献   

三维激光扫描技术下的规划验收测量数据处理及成果获取     

王芬  徐炳前  郝旦 《测绘通报》2019,(4):159-161

三维激光扫描技术由于可快速获取高精度、高密度点云数据,可将拟验收建筑及周边情况几乎完全无差地复制到电脑中,是规划验收测量特别是复杂建筑规划验收测量的理想方法,但是其数据处理一直是影响甚至制约其应用的瓶颈。本文简述了规划验收测量要点,以及三维激光扫描点云数据初步处理流程,并针对制作规划验收测量各类图件的不同需求,提出了分别通过直接取线、切片、投影等方法制作成果图件的工作思路及各方法的特点。但是还需研究和解决海量点云的数据处理,以及根据验收测量特点获得测量成果图件的问题。  相似文献   

利用GLAS激光测高数据评估DSM产品质量及精度优化   总被引：2，自引：0，他引：2  

胡柳茹  唐新明  李国元  付冬暇  窦显辉  赵世湖 《测绘通报》2019,(11):39-43

提出了一种利用卫星激光测高数据直接优化提升数字表面模型（DSM）产品精度的方法。选取境外中亚地区的资源三号DSM开展试验,通过采用多准则约束方法提取激光高程控制点,分别利用偏度、中值、线性、二次多项式等进行DSM误差修正,发现4种模型均能有效消除DSM系统误差,其中基于二次多项式的方法更适用于平地和丘陵地貌,线性模型更适用于高山地貌。试验验证了采用卫星激光测高数据优化境外DSM技术流程的可行性,最终可提高DSM的绝对高程精度。  相似文献   

徕卡RTC360三维激光扫描仪在竣工测量中的应用     

汪晓慧  吴晓培 《测绘通报》2019,(10):150-154,159

徕卡RTC360不仅操作简单、扫描速度快,而且非常智能。可以实时跟踪计算两个连续站点间的相对位置,点云实时预拼接。后期搭配Register360智能拼接软件,点云智能拼接处理,无需人工干预,简单高效。  相似文献   

新型移动三维激光扫描技术在盾构管片椭圆度检测中的应用     

李军  高涛 《测绘通报》2019,(12):159-162

铁运营阶段对隧道结构的变形监测保证了地铁运行的安全,而椭圆度检测是地铁隧道结构检测的重要工作。本文简单介绍了传统椭圆度检测的基本方法,分析了新型移动三维激光扫描检测系统基本原理及隧道椭圆度检测的方法和处理流程。通过工程案例实际应用以及对检测结果的综合分析,证明了移动三维激光扫描技术在盾构管片椭圆度检测中的优势。  相似文献   

差分层析SAR技术研究现状分析     

张月  庞蕾  徐西桂  张天  张瑞菊 《测绘通报》2019,(1):5-12

差分层析SAR是在层析SAR基础上发展起来的一种四维信息反演技术。它不仅实现了对雷达目标的三维分辨能力,同时可以获取目标的形变速率信息,可实现对目标方位-距离-高度-时间四维成像,这对实现城市基础设施动态形变监测、古建筑风险评估、重要工程安全监测等应用具有重要实际意义和价值。本文基于差分层析SAR成像原理,分析了成像处理过程中存在的问题,总结了差分层析SAR成像算法研究现状和特点;最后列举了差分层析SAR技术的主要应用领域,并对其技术发展趋势进行了展望。  相似文献   

基于SSW点云数据的矢量地图平面精度自动校验方法     

羌鑫林  李广伟  王留召  张伟红 《测绘通报》2019,(3):98-102

常规的矢量地图精度校验采用抽样与实地测量,外业工作量大,自动化程度低。针对这一问题,本文提出基于SSW激光点云数据的矢量地图平面精度自动校验方法。首先,使用车载激光扫描器获得道路两侧高精度点云数据,并对点云数据进行滤波、坐标转换和精度检验;其次,基于多特征识别算法,使用SWDY软件提取点云特征点线;最后,利用最近邻法搜索待检矢量图中的同类地物特征点线,并计算匹配点线对的中误差。以兴化城区为试验区,采用该方法检测该地区1：1000比例尺的矢量地图平面精度,试验结果显示,成功匹配了点云数据205个地物特征中的201个,矢量地图的总体中误差为0.26 m,且能够发现待检测矢量地图中的采集丢漏与明显错误。本文方法可以减少现有检测方法的野外实测工作量,增加检测样本数量,降低检测过程中的人为干扰因素,有效提升检测的可靠性与检测效率。  相似文献   

运用人工鱼群算法的3D扫描碎片重建探究     

刘恩盛  程效军  黄玉花 《测绘通报》2019,(3):137-140

针对传统三维碎片拼接匹配过程中依赖单一特征及存在误差累积的问题,提出了一种运用鱼群算法的全局最优匹配方法。该方法先对碎片点云数据进行多特征提取,结合纹理、专家经验信息对混合在一起的多种类型碎片进行粗糙集分类,之后采用鱼群算法的最优解求得最佳匹配方案。实例验证所提全局匹配方法具有能力强、与初始位置无关及较强的稳健性等特点,为三维碎片的全局匹配提供了一种有效的解决方案。  相似文献