Eclipsing Binaries Showing Light–Time Effect     

Petr Zasche 《Astrophysics and Space Science》2005,296(1-4):127-130

Four eclipsing binaries, which show apparent changes of period, have been studied with respect to a possible presence of the light–time effect. With a least squares method we calculated new light elements of these systems, the mass function of the predicted third body, and its minimum mass. We discuss the probability of the presence of such bodies in terms of mass function, changes in radial velocity and third light in solution of light curves.  相似文献   

倾斜矢量图正常年变化破坏的机理研究     

何翔 《大地测量与地球动力学》1993,(1)

根据云南省楚雄、永胜台的倾斜矢量图在强震前正常年变化被破坏的事实,探讨了矢量图面积异常与地震的关系。认为矢量图所围面积的变化与地下水的作用固然有一定的关系,而起决定作用的是地震前应变积累的程度。倾斜矢量图面积的减小可以作为预报的一项参考指标。  相似文献   

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   总被引：2，自引：2，他引：0       下载免费PDF全文

张 艳韩润生  魏平堂邱文龙 《中国地质》2015,(2):607-620

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。  相似文献   

http://www.sciencedirect.com/science/article/pii/S1674987114000401     

Emilio Saccani 《地学前缘(英文版)》2015,6(4)

In this paper, a new discrimination diagram using absolute measures of Th and Nb is applied to post-Archean ophiolites to best discriminate a large number of different ophiolitic basalts. This diagram ...  相似文献   

A comprehensive CCD photometric study of the open cluster NGC 2421     

R. K. S. Yadav  Ram Sagar 《Monthly notices of the Royal Astronomical Society》2004,351(2):667-675

  相似文献   

A 2dF survey of the Small Magellanic Cloud     

Christopher J. Evans  Ian D. Howarth  Michael J. Irwin  Adam W. Burnley  Timothy J. Harries 《Monthly notices of the Royal Astronomical Society》2004,353(2):601-623

  相似文献   

Hipparcos后的昴星团距离     

王家骥  陈力 《天文学进展》2005,23(4):293-303

详细介绍了Hipparcos测定的昴星团距离与以往地面测定结果比较所出现的差异、近年来对昴星团距离新的测定和对Hipparcos数据作的重新处理以及对造成不一致的原因所进行的探讨，最后对有关进展加以评述。  相似文献   

WIYN Open Cluster Study – XVI. Optical/infrared photometry and comparisons with theoretical isochrones     

Aaron J. Grocholski  Ata Sarajedini 《Monthly notices of the Royal Astronomical Society》2003,345(3):1015-1029

We present combined optical/near-infrared photometry ( BVIK ) for six open clusters – M35, M37, NGC 1817, NGC 2477, NGC 2420 and M67. The open clusters span an age range from 150 Myr to 4 Gyr and have metal abundances from  [Fe/H]=−0.27  to +0.09 dex. We have utilized these data to test the robustness of theoretical main sequences constructed by several groups as denoted by the following designations – Padova, Baraffe, Y², Geneva and Siess. The comparisons of the models with the observations have been performed in the  [ M_V , ( B − V )₀], [ M_V , ( V − I )₀]  and  [ M_V , ( V − K )₀]  colour–magnitude diagrams as well as the distance-independent  [( V − K )₀, ( B − V )₀]  and  [( V − K )₀, ( V − I )₀]  two-colour diagrams. We conclude that none of the theoretical models reproduces the observational data in a consistent manner over the magnitude and colour range of the unevolved main sequence. In particular, there are significant zero-point and shape differences between the models and the observations. We speculate that the crux of the problem lies in the precise mismatch between theoretical and observational colour–temperature relations. These results underscore the importance of pursuing the study of stellar structure and stellar modelling with even greater intensity.  相似文献   

Properties of iron at the Earth's core conditions   总被引：2，自引：0，他引：2  

Orson L. Anderson 《Geophysical Journal International》1986,84(3):561-579

Summary. The phase diagram of iron up to 330 GPa is solved using the experimental data of static high pressure (up to 11 GPa) and the experimental data of shock wave data (up to 250 GPa). A solution for the highest triple point is found ( P = 280 GPa and T = 5760 K) by imposing the thermodynamic constraints of triple points. This pressure of the triple point is less than the pressure of the inner core–outer core boundary of the Earth. These results indicate that the density of iron at the inner core–outer core boundary pressure is close to 13 g cm⁻³, which lies close to the seismic solutions of the Earth at that pressure. It is thus concluded that the Earth's inner core is very likely to be virtually pure iron in its hexagonal close packed (hcp) phase.
It is shown that four properties of the Earth's inner core determined from seismology are close in value to the corresponding properties of hcp iron at inner core conditions: density, bulk modulus, longitudinal velocity, and Poisson's ratio. The density–pressure profile of hcp iron at inner core conditions matches the density–pressure profile of the inner core as determined by seismic methods, within the spread of values given by recent seismic models.
This indicates that the Earth is slowly cooling, the Earth's inner core is growing by crystallization, and the impurities of the core are concentrated in the outer core. The calculated temperature at the Earth's centre is 6450 K.  相似文献   

SDINS/GPS in-flight alignment using GPS carrier phase rate     

Joon?Goo?Park  Jang?Gyu?Lee  Chan?Gook?ParkEmail author 《GPS Solutions》2004,8(2):74-81

The alignments of the strapdown inertial navigation system (SDINS) utilizing GPS carrier phase rate measurements is introduced. In this paper, a measurement model of GPS carrier phase rate under two antenna configurations is derived in order to be used for the SDINS alignment process. For in-flight alignment, the performance of the proposed SDINS/GPS integration method is analyzed using the covariance analysis and the overall performance is briefly confirmed by the navigation result of a van test. Furthermore, we find that during in-flight alignment the proposed SDINS/GPS integrated system using GPS carrier phase rate measurements can be implemented in real time because the integer ambiguity problem resulting from carrier phase measurements is avoided.  相似文献