Velocity Curve Analysis of Spectroscopic Binary Stars AI Phe, GM Dra, HD 93917 and V502 Oph by Nonlinear Regression     

K. Karami R. Mohebi 《中国天文和天体物理学报》2007,7(4):558-564

We introduce a new method to derive the orbital parameters of spectroscopic bi-nary stars by nonlinear least squares of (o-c). Using the measured radial velocity data of the four double lined spectroscopic binary systems, AI Phe, GM Dra, HD 93917 and V502 Oph, we derived both the orbital and combined spectroscopic elements of these systems. Our numerical results are in good agreement with the those obtained using the method of Lehmann-Filhe's.  相似文献   

安徽中南部下二叠统栖霞组和孤峰组沉积环境及成岩历史     

朱同兴 《成都地质学院学报》1990,17(1):5-12

皖中南地区下二叠统发育8种不同的沉积相带。栖霞组下部主要发育滨岸细碎屑岩相带和半局限海台地相带，中上部发育开阔海台地相带、较深水台凹相带和台棚内带；早中孤峰期发育台棚外带、台棚内带和台地边缘缓坡相带，晚孤峰期在宿松地区发育了台地边缘生物滩相带，研究区下二叠统成岩环境划为海底-浅埋藏、中埋藏、深埋藏和表生成岩环境，并阐述了这4种成岩环境内的成岩作用类型组合标志。  相似文献   

Stellar and HI Mass Functions Predicted by a Simple Preheating Galaxy Formation Model     

Zhi-Jian Luo Cheng-Gang Shu 《中国天文和天体物理学报》2007,7(4):590-594

According to the new preheating mechanism of galaxy formation suggested by Mo et al., we construct a simple model of formation of disk galaxies within the current paradigm of galaxy formation. It incorporates preheating, gas cooling, bulge formation and star for-mation. The predicted stellar and HI mass functions of galaxies are discussed and compared with the observations. It is found that our model can roughly match both the observed galaxy luminosity function and the observed HI-mass function.  相似文献   

CO Clouds around SNR G21.8-0.6 and G32.8-0.1     

Jian-Jun Zhou Xi-Zheng Zhang Hong-Bo Zhang Jarken Esimbek Ju-Yong Zhang Bing-Gang Ju 《中国天文和天体物理学报》2007,7(5):705-711

We made the first CO(I—0) mapping to SNR G21.8-0.6 and SNR G32.8-0.1, both associated with OH 1720 MHz maser.Based on the morphological correspondence and velocity and position agreement between the radio remnant and the CO clouds,we tentatively identify the clouds that are respectively interacting with the two SNRs.  相似文献   

A Survey of Newtonian Core-Shell Systems with Pseudo High Order Symplectic Integrator and Fast Lyapunov Indicator     

Jun-Fang Zhu Xin Wu Da-Zhu Ma 《中国天文和天体物理学报》2007,7(4):601-610

Newtonian core-shell systems, as limiting cases of relativistic core-shell models under the two conditions of weak field and slow motion, could account for massive circumstellar dust shells and rings around certain types of star remnants. Because this kind of systems have Hamiltonians that can be split into a main part and a small perturbing part, a good choice of the numerical tool is the pseudo 8th order symplectic integrator of Laskar ＆ Robutel, and, to match the symplectic calculations, a good choice of chaos indicator is the fast Lyapunov indicator （FLI） with two nearby trajectories proposed by Wu, Huang ＆ Zhang. Numerical results show that the FLI is very powerful when describing not only the transition from regular motion to chaos but also the global structure of the phase space of the system.  相似文献   

Disk Thicknesses and Some Parameters of 108 Non-Edge-On Spiral Galaxies     

Tao Hu Qiu-He Peng Hong-Shi Zong 《中国天文和天体物理学报》2007,7(4):579-589

We present disk thicknesses, some other parameters and their statistics of 108 non-edge-on spiral galaxies. The method for determining the disk thickness is based on solving Poisson's equation for a disturbance of matter density in three-dimensional spiral galaxies. From the spiral arms found we could obtain the pitch angles, the inclination of the galactic disk, and the position of the innermost point (the forbidden region with radius r 0 to the galactic center) of the spiral arm, and finally the thickness.  相似文献   

湘南五峰仙岩体γ能谱区调成果分析     

沈赵明  颜小莲 《湖南地质》2009,(5):74-76

应用γ能谱测量成果，从分析岩体含铀性、古铀参数特征入手，进一步总结了铀、钍、钾晕及铀异常显示特征，并对五峰仙岩体铀成矿前景进行了预测。  相似文献   

水城放区龙潭组浅绿色泥岩的特征及成因     

陈荣舟 《煤田地质与勘探》1990,(1):17-20

  相似文献   

辽河盆地东部凹陷古近系沙河街组层序地层及沉积相研究     

《东北石油大学学报》2015,(6)

根据岩心、测井和地震资料综合分析结果,研究辽河盆地东部凹陷沙河街组层序地层划分、沉积相类型及展布特征,东部凹陷沙河街组层序地层格架中识别出3个三级层序界面(SB1、SB2和SB3),划分2个三级层序(SQ1和SQ2);识别出冲积扇相、扇三角洲相、辫状河三角洲相、浊积扇相和湖泊相等沉积相类型.基于层序地层格架的划分和层序格架沉积砂体的特征研究,结合岩心相、测井相及地震相分析,绘制东部凹陷沙河街组不同层序的沉积相平面展布图.根据东部凹陷沙河街组沉积相空间展布及演化规律,结合沉积相分布控制因素分析,提出东部凹陷沙河街组沉积相模式,盆地陡坡带短距离搬运的沉积物质在陆上堆积形成冲积扇,进入水体发育扇三角洲、浊积扇体等;缓坡带沉积物搬运距离相对较远,多发育辫状河—辫状河三角洲等远源沉积体系.  相似文献   

琼东南盆地深水区中央峡谷黄流组物源特征   总被引：3，自引：2，他引：1  

左倩媚  张道军  何卫军  王亚辉  王真真  陈杨 《海洋学报》2015,37(5):15-23

物源分析作为岩相-古地理研究的前提和基础,物源体系决定了砂体的展布和储集性能。为明确中央峡谷体系黄流组储集体展布规律及下一步勘探方向,本文应用中央峡谷最新钻井资料,采用重矿物组合、锆石U-Pb测年等分析方法,结合地震反射特征,对中央峡谷黄流组物源体系特征进行分析。地震反射特征表明来自海南隆起和昆嵩隆起物源的三角洲体系,通过二次搬运沉积了陆架斜坡区和盆底的低位海底扇,为中央峡谷的沉积充填提供了充足的粗碎屑沉积物;新钻井黄流组样品中重矿物组合以白钛矿、石榴石、磁铁矿含量较高为主要特征,与莺歌海盆地受蓝江物源影响和琼东南盆地受丽水-秋滨河物源影响的地层重矿物组合相似;锆石U-Pb测年分析表明,中央峡谷黄流组地层中样品年龄图谱具有30~2 000Ma变化范围,与莺歌海盆地受昆嵩隆起物源影响的钻井以及越南现代河流采集的沙样具有非常一致的年龄段和丰度。综上所述,中央峡谷受多物源的影响,越南昆嵩隆起为主的琼东南盆地西部物源体系,是琼东南盆地乐东凹陷晚中新世深水扇以及中央峡谷粗碎屑物质的主要沉积物供给来源区。  相似文献