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Jun-Liang Zhao Li Chen 《中国天文和天体物理学报》2007,7(4):572-578
On the reasonable hypothesis that the internal motions of member stars of a cluster are random and isotropic, a method which can be used to estimate the velocity distance of the cluster and its uncertainty is developed. The velocity distance so determined is an absolute distance estimate, and is completely independent of the (widely used) luminosity distance, which is a relative distance estimate. Using the published high-accuracy observational data of radial velocities and proper motions of the stars in the open cluster M11 region, we have determined the distance of M11 to be 1.89 ± 0.52kpc. This is in quite good agreement with the published luminosity distances of the cluster. We briefly discuss the problems concerned, including the sources of errors in the method and its applicable range. 相似文献
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Jun-Liang Zhao Li Chen Wen Wen Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai Shanghai University Shanghai 《中国天文和天体物理学报》2006,6(4):435-446
From photographic plate data of Shanghai Astronomical Observatory with a time baseline of 87 years, proper motions and membership probabilities of 364 stars in the open cluster NGC 6530 region are reduced. On the basis of membership determination, luminosity function and segregation effect of the cluster are discussed with details. Spatial mass segregation is obviously present in NGC 6530 while there is no clear evidence for a velocity-mass (or velocity-luminosity) dependence. The observed spatial mass segregation for NGC 6530 might be due to a combination of initial conditions and relaxation process. 相似文献
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Jun-Liang Yuan Jin-Gen Deng Qiang Tan Bao-Hua Yu Xiao-Chun Jin 《Rock Mechanics and Rock Engineering》2013,46(5):1157-1164
Serious wellbore instability occurs frequently during horizontal drilling in shale gas reservoirs. The conventional forecast model of in situ stresses is not suitable for wellbore stability analysis in laminated shale gas formations because of the inhomogeneous mechanical properties of shale. In this study, a new prediction method is developed to calculate the in situ stresses in shale formations. The pore pressure near the borehole is heterogeneous along both the radial and tangential directions due to the inhomogeneity in the mechanical properties and permeability. Therefore, the stress state around the wellbore will vary with time after the formation is drained. Besides, based on the experimental results, a failure criterion is verified and applied to determine the strength of Silurian shale in the Sichuan Basin, including the long-term strength of gas shale. Based on this work, horizontal well borehole stability is analyzed by the new in situ stress prediction model. Finally, the results show that the collapse pressure will be underestimated if the conventional model is used in shale gas reservoirs improperly. The collapse pressure of a horizontal well is maximum at dip angle of 45°. The critical mud weight should be increased constantly to prevent borehole collapse if the borehole is exposed for some time. 相似文献
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广州飞龙世界游乐城关闭的原因与启示 总被引：2，自引：1，他引：2
广州番禺“飞龙世界游乐城”是广州市首座主题公园，在1995年元月开业前后，各种新闻媒体普作过大量宣传，实际景点建设、经营运作声势浩大，一度名扬粤港澳，但在营业4年后，却被广州番禺法院封闭停业了。文中从旅游科学和旅游业实践的角度，通过实地调查研究，认为其失败的主要原因是：（1）景点建设背离主题，贪大求全；（2）市场定位盲目乐观，大量设施空置；（3）经营管理上未能扬长避短，蛇系列产品未能适销对路进入园国际市场；（4）投资机制上靠贷款建设，经营严重亏损，并从中得到几点启迪，供今后创办主题公园借鉴。 相似文献
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Jun-Liang Zhao Li Chen Zhong-Liang Zu Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai 《中国天文和天体物理学报》2006,6(3):287-296
Absolute proper motions and radial velocities of 202 open clusters in the solar neighborhood, which can be used as tracers of the Galactic disk, are used to investigate the kinematics of the Galaxy in the solar vicinity, including the mean heliocentric velocity components (u_1,u_2,u_3) of the open cluster system, the characteristic velocity dispersions (σ_1,σ_2,σ_3), Oort constants (A, B) and the large-scale radial motion parameters (C,D) of the Galaxy. The results derived from the observational data of proper motions and radial velocities of a subgroup of 117 thin disk young open clusters by means of a maximum likelihood algorithm are: (u_1,u2,u3) = (-16.1±1.0, -7.9±1.4,-10.4±1.5) kms~(-1), (σ_1,σ_2,σ_3) = (17.0 ±0.7,12.2±0.9,8.0±1.3) kms~(-1),(A,B) = (14.8±1.0,-13.0±2.7) kms~(-1) kpc~(-1) ,and(C,D) = (1.5±0.7,-1.2±1.5) kms~(-1) kpc~(-1) . A discussion on the results and comparisons with what was obtained by other authors is given. 相似文献
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湖南七宝山石英斑岩地球化学特征及其与成矿的关系 总被引：1，自引：0，他引：1
湖南浏阳七宝山铜多金属矿床位于钦杭成矿带西南段,是湘东北规模最大的铜多金属矿床,其中矿区内的石英斑岩对成矿贡献非常大。七宝山矿区的石英斑岩是一套高钾(K2O>>Na2O)、富铝、贫硅的亚碱性的粗面安山岩—安山岩—英安岩组合,地球化学上显示了富轻稀土(LREE)、大离子亲石元素(LILE)(Ba,K等)、成矿元素(Cu、Pb、Zn等),以及贫重稀土元素(HREE)特征。稀土元素配分模式为右倾,有轻微的Eu负异常,说明它具有部分幔源特征;而明显的Sr负异常,且与地壳丰度相似,加上较高Al2O3/TiO2、K2O/Na2O比值,投图后均显示岩石为地壳来源。综合上述特征本文认为该石英斑岩属壳幔同熔型花岗岩。矿体与岩体在空间、时间上关系密切,岩体很高的成矿元素含量正是形成矿体的物质来源。其作用过程是岩浆作为载体携带成矿元素从地幔到近地表,并且在各种导矿构造作用下充填交代成矿。 相似文献