Conservative two-body problem with variable masses     

L. G. Luk’yanov 《Astronomy Letters》2005,31(8):563-568

We consider the conservative two-body problem with a constant total mass, but with variable individual masses. The problem is shown to be completely integrable for any mass variation law. The Keplerian motion known for the classical two-body problem with constant masses remains valid for the relative motion of the bodies. The absolute motions of the bodies depend on the center-of-mass motion. Hitherto unknown quadratures that depend on the mass variation law were derived for the integrals of motion of the center of mass. We consider some of the laws that are of interest in studying the motion of close binary stars with mass transfer.  相似文献   

In between β Lyrae and Algol: The Case Of V356 Sgr     

D. Dominis  P. Mimica  K. Pavlovski  E. TAMAJO 《Astrophysics and Space Science》2005,296(1-4):189-192

The eclipsing binary system V356 Sgr is of considerable interest, since it is probably at the very end of its mass transfer phase, i.e. between β Lyrae and Algol. Hence, the binary provides an opportunity to directly examine the exposed core of a star for signatures of nuclear burning, and to test stellar evolution models. The system is composed of an early B star accreting matter from a Roche-lobe filling A2 II star. Recently, with progress in the UV spectral region, significant revision of previous values for absolute parameters has been made. Therefore, we find it justified and important to present a new photometric solution. Our model is compared to an early disk model, and is discussed in the framework of mass transfer processes in this binary system.  相似文献   

The X-ray intensity-hardness ratio relation in LMXRB     

Krishna M. V. Apparao  S. P. Tarafdar 《Journal of Astrophysics and Astronomy》1993,14(3-4):135-139

It is sometimes suggested that the change from the horizontal to the normal branch in the X-ray intensity-hardness ratio diagram of low mass X-ray binaries, is due to a change from a thin to a thick disk. It is shown here that wind from the hot thick disk depletes the amount of matter reaching the neutron star, thus causing the observed reduction of X-ray intensity as hardness ratio decreases in the normal branch.  相似文献   

密近双星的测光研究     

《天文研究与技术》1997,(1)

  相似文献   

徕卡全站仪GSI数据格式转换模块设计     

岳超 《安徽地质》2015,(1):73-75

基于全站仪的数字测图是获取地理空间信息数据的重要手段,由于全站仪品牌不同,其数据格式区别较大,且不能直接导入到成图软件中。本文对徕卡系列全站仪数据存储所采用的GSI-8格式进行了分析,介绍了GSI-8转CASS7.0所需的*.dat格式的原理,给出了程序实现的核心代码,利用实例数据对数据格式转换模块进行了验证。本文所介绍的文件格式转换方法对于测量中其它数据格式的转换具有一定的参考意义。  相似文献   

S-57等深线数据的格式转换与集成     

高敏  罗毅  张景发  杨建钦 《测绘工程》2015,(5)

以中国海区501幅42种比例尺的等深线图为例,将其S-57格式转换为shp格式,并通过ArcGIS平台进行批处理合并。在先验知识和其他图层的参与下,分别制定不同的处理原则,实现所有比例尺的等深线在同一比例尺下显示。  相似文献   

多核并行环境中矢量数据格式的转换算法   总被引：1，自引：0，他引：1  

周琛  陈振杰  黄秋昊  黄涛 《测绘科学》2015,40(7)

针对目前对VCT格式转换的并行算法研究较少的现状,该文以VCT向shapefile格式转换为例,探索多核并行环境中进行VCT格式向其他矢量数据格式快速转换的方法:在深入探索VCT与shapefile格式特点的基础上,通过构建索引、数据解析转换,完成由VCT向shapefile格式的转换;并设计出一种顾及负载均衡的数据划分方法,通过评估不同类型图层的复杂度实现不同类型矢量数据的均衡划分,实现了VCT向shapefile格式转换的并行算法。最后利用某地土地利用VCT文件进行算法测试,结果表明该算法转换结果正确,取得了良好的加速比,并基本达到负载均衡。  相似文献   

基于全天空极光图像方向能量表征方法的极光事件分类          下载免费PDF全文

张军 胡泽骏王倩  梁继民 《极地研究》2015,27(3):255-263

针对基于全天空极光图像的极光事件自动分类问题,提出一种基于方向能量二元编码重组表征的自动分类方法。首先,通过对多个方向上能量分解来描述极光事件中的局部纹理和各个方向上的运动信息,并且结合分块策略获得极光事件的全局形态信息;然后,借鉴一种二元编码重组的方式对多个方向能量进行融合,从而使得极光事件的表征具有同时表征局部纹理、全局形态和运动信息的能力。该表征方法完全不依赖于极光事件的长度,可用于表征不同持续时间的极光事件,并且不需要复杂的训练过程。利用最近邻和支撑向量机分类器分别对从中国北极黄河站拍摄到的极光图像中挑选的特定极光事件进行自动分类,结果表明,与其他两种典型的动态纹理描述方法相比,本文所提出的表征方法结合最近邻分类器,得到了最好的分类效果,能有效用于极光事件的分析,为海量数据中的极光事件自动分类提供了一种新方法。  相似文献   

Pleiades卫星图像正射纠正方法     

杨宝林  吕婷婷  王少军  张志 《国土资源遥感》2015,(3)

Pleiades卫星图像是一种应用时间尚短的新型遥感图像,目前还缺少对其专用的正射纠正处理方法。为此,以湖北省大冶—阳新地区的6景Pleiades图像为例,在Visual Studio 2008环境下,采用C#语言开发了针对Pleiades图像有理多项式系数(rational polynomial coefficients,RPC)文件格式的转换软件包,用于将Pleiades图像的RPC文件格式转换为IKONOS图像的RPC文件格式,并采用ERDAS9.2中的IKONOS图像的正射纠正模型对其进行纠正。该方法解决了对Pleiades图像进行正射纠正所需要解决的相关问题,开发的RPC文件转换程序可以用于批量的Pleiades卫星RPC文件格式转换,提高了转换效率和准确性,为大规模应用Pleiades图像奠定了基础。  相似文献   

Light-Time Effect in the Eclipsing Binaries GO Cyg, GW Cep, AR Aur and V505 Sgr     

D. Chochol  T. Pribulla  M. Vaňko  P. Mayer  M. Wolf  P. G. Niarchos  K. D. Gazeas  V. N. Manimanis  L. Brát  M. Zejda 《Astrophysics and Space Science》2006,304(1-4):93-96

Orbital period changes of the eclipsing binaries GO Cyg and GW Cep are explained by the light-time effect for the first time. New minima of the eclipsing binary AR Aur improve the predicted light-time orbit. The light-time orbit with the quadratic ephemeris of the binary matches the new observations of V505 Sgr better than the linear one. As the light-time effect fits in corresponding O − C diagrams of all four systems have been reaching extreme values, the observations of minima times in forthcoming years are highly desirable.  相似文献