准噶尔盆地车排子隆起西南部原油地球化学特征及油源分析   总被引：6，自引：3，他引：3  

张枝焕  李伟  孟闲龙  秦黎明  张振英  袁东山 《现代地质》2007,21(1):133-140

车排子隆起毗邻昌吉凹陷和四棵树凹陷,油源丰富,构造条件良好,具备比较有利的油气聚集条件。近年来已在车排子隆起的侏罗系、白垩系、古近系和新近系获高产工业油气流。分析了车排子隆起西南部原油（或油砂抽提物）的地球化学特征,并对其油源作初步分析。结果表明研究区具有两类地球化学性质存在明显差别的原油。第一类原油遭受了不同程度的生物降解,并存在二次充注现象,推测早期充注原油来自昌吉凹陷二叠系,并遭受了不同程度的生物降解,后期混入了来自侏罗系烃源岩生成的原油。第二类原油具有侏罗系煤系烃源岩与白垩系湖相泥质烃源岩混源的特点,这类原油的碳同位素组成、正构烷烃分布特征和姥植比等均表现出煤成油的特征,但甾、萜烷烃类化合物组成与白垩系烃源岩接近,推测是由于侏罗系煤成油在向上运移成藏过程中,受到成熟度相对较低、生物标志物相对丰富的白垩系烃源岩的浸析作用所致。  相似文献   

Stellar sources in the isogal inner galactic bulge field (l=0°,b= − 1°)     

D. K. Ojha  A. Omont  S. Ganesh  G. Simon  M. Schultheis 《Journal of Astrophysics and Astronomy》2000,21(1-2):77-90

ISOGAL is a survey at 7 and 15 μm with ISOCAM of the inner galactic disk and bulge of our Galaxy. The survey covers ∼ 22 deg² in selected areas of the centrall = ±30 degree of the inner Galaxy. In this paper, we report the study of a small ISOGAL field in the inner galactic bulge (l = 0°,b = −1°, area = 0.033deg²). Using the multicolor nearinfrared data (IJK_s) of DENIS (DEep Near Infrared Southern Sky Survey) and mid-infrared ISOGAL data, we discuss the nature of the ISOGAL sources. The various color-color and color-magnitude diagrams are discussed in the paper. While most of the detected sources are red giants (RGB tip stars), a few of them show an excess in J-K_s and K_s-[15] colors with respect to the red giant sequence. Most of them are probably AGB stars with large mass-loss rates.  相似文献   

基坑潜在隆起破裂面的Dijkstra组合优化搜索法     

胡志平  姚海明  罗丽娟 《岩土力学》2006,27(9):1583-1587

运用弹塑性有限元程序计算基坑围护结构与土体任意一点在开挖前后的应力状态,根据选定的屈服准则计算其极限状态函数值,通过有限元网格节点及其坐标,采用“人机对话”的优化方法选择坑底最大可能的隆起破裂面的起点和终点,通过Dijkstra算法找出基坑土体最可能发生坑底隆起破坏的潜在破裂面的形状及位置,并求出相应的安全系数。大量数值计算和实测资料表明：潜在破裂面终点的位置对围护桩插入比不敏感,而潜在破裂面起点位置则随围护桩入土深度的增加而逐渐靠近围护桩。搜索法得到的潜在破裂面突破了以往人为给定破裂面形状和极限土压力假定的限制,工程算例证实了基于组合优化Dijkstra算法的潜在破裂面搜索法的有效性和实用性。  相似文献   

脉动变星数据库的建立     

陈丙秋  杨明  姜碧沩 《天文学报》2011,52(4)

为了方便国内学者对脉动变星进行研究,建立了一个数据库,目前包含了时间长达10 yr左右的巡天项目MAssive Compact Halo Objects(大质量致密银晕天体,MACHO)和Optical Gravitational Lensing Experiment(光学引力透镜实验,OGLE)发现的脉动变星,一共容纳了来自银河系核球与大小麦哲伦云中的共近23万颗变星.采用的软件是LAMP,即Linux+Apache+MySQL+PHP.数据库的使用通过网页的简单搜索界面实现,搜索参数主要是天体的赤经、赤纬和半径.鉴于本数据库的灵活性,将来很方便加入其他的变星数据.  相似文献   

Parallax microlensing events in the OGLE II data base toward the Galactic bulge     

Martin C. Smith  Shude Mao  P. Woz´niak 《Monthly notices of the Royal Astronomical Society》2002,332(4):962-970

We present a systematic search for parallax microlensing events among a total of 512 microlensing candidates in the OGLE II data base for the  1997–1999  seasons. We fit each microlensing candidate with both the standard microlensing model and a parallax model that accounts for the Earth's motion around the Sun. We then search for the parallax signature by comparing the χ ² of the standard and parallax models. For the events which show a significant improvement, we further use the 'duration' of the event and the signal-to-noise ratio as criteria to separate true parallax events from other noisy microlensing events. We have discovered one convincing new candidate, sc33_4505, and seven other marginal cases. The convincing candidate (sc33_4505) is caused by a slow-moving, and likely low-mass, object, similar to other known parallax events. We found that irregular sampling and gaps between observing seasons hamper the recovery of parallax events. We have also searched for long-duration events that do not show parallax signatures. The lack of parallax effects in a microlensing event puts a lower limit on the Einstein radius projected on to the observer plane, which in turn imposes a lower limit on the lens mass divided by the relative lens–source parallax. Most of the constraints are however quite weak.  相似文献   

Proper motion dispersions of red clump giants in the galactic bulge: observations and model comparisons     

Nicholas J. Rattenbury  Shude Mao  Victor P. Debattista  Takahiro Sumi  Ortwin Gerhard  Flavio De Lorenzi 《Monthly notices of the Royal Astronomical Society》2007,378(3):1165-1176

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M giants in MACHO, DENIS and ISOGAL     

I. S. Glass  M. Schultheis 《Monthly notices of the Royal Astronomical Society》2002,337(2):519-528

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Optical gravitational lensing experiment: OGLE-1999-BUL-19 – the first multipeak parallax event     

Martin C. Smith  Shude Mao  P. Wo&#;niak  A. Udalski  M. Szyma&#;ski  M. Kubiak  G. Pietrzy&#;ski  I. Soszy&#;ski  K. &#;ebru&#; 《Monthly notices of the Royal Astronomical Society》2002,336(2):670-684

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Constraints on Jupiters from observations of Galactic bulge microlensing events during 2000     

Yiannis Tsapras †  Keith Horne  Richard Carson  Javier Méndez Alvarez  Dan Batcheldor  Alister W. Graham  Philip A. James  Johan Knapen  Hannah Quaintrell  Ignacio Gonzalez Serrano  Peter Sorensen  Nick Wooder 《Monthly notices of the Royal Astronomical Society》2002,337(1):41-48

We present observations of eight Galactic bulge microlensing events taken with the 1.0-m Jacobus Kapteyn Telescope (JKT) on La Palma during 2000 June and July. The JKT observing schedule was optimized using a prioritizing algorithm to automatically update the target list. For most of these events we have sampled the light curves at times where no information was available from the OGLE alert team. We assume a point-source point-lens (PSPL) model and perform a maximum likelihood fit to both our data and the OGLE data to constrain the event parameters of the fit. We then refit the data assuming a binary lens and proceed to calculate the probability of detecting planets with mass ratio   q = 10⁻³  . We have seen no clear signatures of planetary deviations on any of the eight events and we quantify constraints on the presence of planetary companions to the lensing stars. For two well-observed events, 2000BUL31 and 2000BUL33, our detection probabilities peak at ∼30 and ∼20 per cent respectively for   q = 10⁻³  and   a ∼ R _E  for a  Δχ²  threshold value of 60.  相似文献   

New planetary nebulae in the Galactic bulge region with l > 0°– I. Discovery method and first results     

P. Boumis  †  E. V. Paleologou  F. Mavromatakis  J. Papamastorakis 《Monthly notices of the Royal Astronomical Society》2003,339(3):735-747

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