Conservative two-body problem with variable masses

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.     

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

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.     

The X-ray intensity-hardness ratio relation in LMXRB

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.     

云南昭通铅锌矿pH-logfo_2和pH-loga相图对铅锌共生分异的制约

云南昭通大型铅锌矿是滇东北矿集区乃至川滇黔铅锌成矿域铅锌矿床的典型代表。矿床具有明显的矿物组合分带性的特点,区别于典型的MVT型铅锌矿床。根据矿物组合特征构建、计算、绘制了该矿床的p H-logfo2、p Hloga相图,剖析了铅锌矿共生分异的形成机理。研究表明p H、氧逸度、组分浓度的协同作用造成了铅、锌的共生分异,对矿物组合分带起控制作用,且温度下降、氧逸度升高和p H升高有利于金属硫化物的沉淀,成功解释了昭通铅锌矿床独具特色的矿物分带地质特征。     

一种基于全球剖分网格的多源遥感数据空间关联方法

针对遥感数据具有多源化且数据量大等特征,同时缺乏统一的空间组织框架,对于数据间空间关联关系建立存在困难等问题,文章提出了基于全球剖分网格的多源遥感数据空间关联模型解决方法:首先采用GeoSOT剖分框架对多源遥感数据进行统一组织与管理,然后根据提出的"网格-数据块-数据"的三层组织概念模型,建立基于全球剖分网格的多源遥感数据空间关联模型;最后进行关联影像的表达实验。实验结果表明,该方法在一定程度上实现了多源遥感数据的结构化组织,有效建立了多源遥感数据的空间关联,并与传统的坐标系统建立对比分析,提高了数据利用的应用效能,整体上促进了遥感数据的使用效率。     

基于全天空极光图像方向能量表征方法的极光事件分类

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。     

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

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.     

蓝离散星研究现状(Ⅰ):形成机制

大量研究表明,蓝离散星的形成可能有多种机制,目前比较流行的形成机制可以概括为以下几类:密近双星系统的质量传输及双星并合、密集星场的恒星碰撞,以及包含双星系统的恒星间 (双星-单星、双星-双星)相互作用导致的恒星并合。与此同时,蓝离散星在各类恒星系统中的普遍存在,也使得研究这类恒星的形成及演化成为追踪恒星系统动力学演化、化学演化及积分光谱性质变化的有效指针。     

蓝离散星研究现状(Ⅱ):观测特性

不同恒星系统(银河系晕、疏散星团、球状星团、矮星系)中蓝离散星所表现出的观测特性各不相同,这与恒星系统动力学环境及相应的蓝离散星主导形成机制直接相关。因此,分析研究蓝离散星的不同观测特性,也就成为研究蓝离散星形成机制、恒星及双星系统演化以及恒星系统动力学演化的有效方法。