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   

More than two hundred and fifty thousand spectroscopic binary or variable star candidates discovered by LAMOST     

Sheng-Bang Qian  Xiang-Dong Shi  Li-Ying Zhu  Lin-Jia Li  Jia Zhang  Er-Gang Zhao  Zhong-Tao Han  Xiao Zhou  Xiao-Hui Fang  Wen-Ping Liao 《天文和天体物理学研究(英文版)》2019,(5):15-26

About 786.4 thousand stars were observed by LAMOST twice or more during the first stage of its spectroscopic survey. The radial velocity differences for about 256 thousand targets are larger than10 km s^-1 and they are possible spectroscopic binary or variable candidates(SBVCs). It is shown that most SBVCs are slightly metal poorer than the Sun. There are two peaks in the temperature distribution of SBVCs around 5760 K and 4870 K, while there are three peaks in the distribution of the gravitational acceleration at 2.461, 4.171 and 4.621 cm s^-2. The locations of SBVCs on the [Fe/H]-T, [Fe/H]-log g, log g-T and H-R diagrams are investigated. It is found that the detected SBVCs could be classified into four groups. The first group has higher log g～4.621 and lower T ～ 4870 K which are mainly cool red dwarf binaries. The second group of SBVCs has logg around 4.171 cm s^-2 that includes binaries and pulsating stars such as δSet and γ Dor variables. The gravitational accelerations of the third group of SBVCs are higher and some of them are below the zero-age main sequence. They may be contact binaries in which the primary components are losing energy to the secondaries in the common envelopes and are at a special stellar evolutionary stage.The last group is composed of giants or supergiants with log g around 2.461 cm s^-2 that may be evolved pulsating stars. One target(C134624.29+333921.2) is confirmed as an eclipsing binary with a period of 0.65 days. A preliminary analysis suggests that it is a detached binary with a mass ratio of 0.46. The primary fills its critical Roche lobe by about 89%, indicating that mass transfer will occur between the two components.  相似文献   

Preface: Modern studies of variable stars     

Nikolay N.Samus  Sheng-Bang Qian 《天文和天体物理学研究(英文版)》2019,(3):1-2

In this Mini-Volume, seven papers written on the basis of talks selected from those presented at the scientific conference "Modern studies of variable stars," commemorating Prof. M. A. Svechnikov(1933–2011), are published. The conference covered a variety of variable-star topics; the papers in this Mini-Volume deal with close, mainly eclipsing, binaries, Herbig Be stars and stellar molecular masers, with an accent on stellar catalogs of different kinds. We briefly review the contents of these papers.  相似文献   

X-ray activity from different types of stars     

Lin He  Song Wang  Xiao-Jie Xu  Roberto Soria  Ji-Feng Liu  Xiang-Dong Li  Yu Bai  Zhong-Rui Bai  Jin-Cheng Guo  Yan-Li Qiu  Yong Zhang  Ruo-Chuan Xu  Ke-Cheng Qian 《天文和天体物理学研究(英文版)》2019,(7)

X-ray emission is an important indicator of stellar activity. In this paper, we study stellar Xray activity using the XMM-Newton and LAMOST data for different types of stars. We provide a sample including 1259 X-ray-emitting stars, of which 1090 have accurate stellar parameter estimations. Our sample size is much larger than those used in previous works. We find a bimodal distribution of the X-ray to optical flux ratio(log(fX/fV)) for G and K stars. We interpret that this bimodality is due to two subpopulations with different coronal heating rates. Furthermore, using the full widths at half maxima calculated from Hα and Hβ lines, we show that these stars in the inactive peaks have smaller rotational velocities. This is consistent with the magnetic dynamo theory that presumes stars with low rotational velocities have low levels of stellar activity. We also examine the correlation between log(fX/fV) and luminosity of the excess emission in the Hα line, and find a tight relation between the coronal and chromospheric activity indicators.  相似文献   

GF-2支持下的干旱区稀疏植被区植被覆盖度估算     

沈谦  朱长明  张新 《测绘通报》2019,(7):33-38

现有像元二分模型MODIS植被覆盖度模型因其形式简单、适用性较强的特点被广泛应用于区域植被覆盖度（FVC）的估算。然而,研究表明在沙漠和低植被覆盖的西部干旱区,从250 m的影像上很难精准地获取NDVI_veg（全植被覆盖植被指数）和NDVI_soil（全裸土区植被指数）参数。利用常用的直方图累计法获取模型所需参数NDVI_veg和NDVI_soil,估算结果存在普遍高估现象。为此,本文首先引入同期获取的GF-2号卫星数据,从GF-2号影像上提取植被覆盖像元;然后,利用Pixel Aggregate方法重采样至250 m分辨率,获取250 m空间分辨率下纯植被和纯裸土像元;最后,将纯植被和纯裸土像元各自空间位置相对应的MODIS NDVI数据最大值作为模型所需NDVI_veg和NDVI_soil参数,实现研究区内植被覆盖度的估算。试验通过与线性回归法、多项式回归法和直方图累计像元二分模型法估算结果进行精度对比,结果表明：利用GF-2影像辅助的像元二分模型,精准地获取了低植被覆盖区NDVI_veg和NDVI_soil模型参数,提高了干旱区植被覆盖度的估算精度,并有效地抑制了受稀疏植被影响NDVI在干旱区普遍偏高问题导致的FVC高估的现象。  相似文献   

Multi-band Solar Full-disk Extreme Ultraviolet Imager     

PENG Ji-long  FENG Tao-jun  SHI En-tao  LI Lin  YU Qian  ZHANG Kai  NIE Xiang-yu  MA Zi-liang 《Chinese Astronomy and Astrophysics》2019,43(3):444-456

Solar Extreme Ultraviolet (EUV) imaging observation is an important measure for the researches of solar activities and coronal plasma physics. But the traditional EUV imager and spectrograph can hardly achieve simultaneously the high spectral resolution and wide field-of-view of solar imaging. This paper has designed a new type of solar EUV multi-band imager, by adopting a kind of slitless grating and grazing incidence structure, it can realize the solar full-disk imaging of high spectral and spatial resolution. The field-of-view of the imager can be as broad as 47′. The spectral resolution is 2×10^?3nm per pixel, and the spatial resolution is 1.4′ per pixel. The temporal resolution of the solar full-disk is better than 60 s. The analysis of the solar full-disk spectral image and system response shows that the imager can observe the morphological evolutions of various solar activities, and can provide more comprehensive data for the researches of solar physics and space weather forecast.  相似文献   

三维实景地图生产与应用     

曹培国  姚磊  李奎英  赵倩 《山东国土资源》2018,34(9)

实景地图近年来发展迅速,在日常生活中应用广泛,如旅游景点、宾馆、银行、政府服务中心等的空间位置查询、服务内容介绍等。实景地图的生产方法、生产流程有多种多样,产品质量参差不齐。目前,利用轻型无人机航空摄影系统实现三维全景地图生产,生产方式方便、高效且质量较好。该文介绍了生产三维实景地图的无人机系统及三维实景地图生产方法与过程,通过采用无人机系统实景地图的生产实例,讲述了实景地图应用现状、发展前景及存在的问题。  相似文献   

D—InSAR三轨法监测城市地表沉降的研究     

胡波  蒋弥  王兴旺  孙倩 《测绘工程》2009,18(2):46-50

差分干涉测量（DInSAR）技术是合成孔径雷达（SAR）卫星应用的一个拓展。雷达图象的差分干涉可用于监测厘米级或更微小的地表形变,以揭示许多物理现象,如地震形变、火山运动、大气变化、冰川漂移、地面沉降以及山体滑坡等。实验选取典型的上海市地面沉降场作为研究对象,使用三幅欧洲空间局ERS1和ERS2的C波段数据,采用三轨法,成功提取了上海市相隔20个月的地面沉降图。  相似文献   

跨海大桥高程基准统一新方法研究   总被引：1，自引：0，他引：1  

花向红  许承权  范千 《测绘工程》2009,18(2)

提出基于高程异常差的GPS跨海水准新方法,给出新方法的基本原理和数据处理方案,对用垂线偏差、神经网络法、支持向量机求解高程异常差方法的精度和实用范围作计算分析.结果表明:基于垂线偏差的高程异常差拟合方法适用于距离约5 km的高程传递.基于支持向量机的高程异常差拟合方法,在平原地区,当GPS和水准重合点的点数较多、点位分布较合理时,跨距可以达到30 km.而基于神经网络进行高程异常差拟合适用于距离约10 km的高程传递.  相似文献   

SESAM锁模激光器在卫星激光测距领域应用研究     

卫志斌  瞿锋  项清革  李谦 《测绘科学》2009,34(6)

本文在分析SESAM(Semiconductor Saturable Absorber Mirrors)锁模激光器原理及技术特点、描述其工作流程的基础上,展示了SESAM锁模激光器用于卫星激光测距的实测结果,通过对卫星激光测距数据数量及质量分析,得出了SESAM锁模激光器以窄脉冲宽度、高能量密度、输出稳定等优势首次在国内应用于卫星激光测距系统后,使系统整体性能得到明显提升的结论。  相似文献