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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The OGLE-II event sc5_2859: an example of disc–disc microlensing     

Martin C. Smith 《Monthly notices of the Royal Astronomical Society》2003,343(4):1172-1180

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安全壳鼓包测量系统的设计及实现     

徐亚明  张宇 《测绘通报》2021,(12):149-152

在核电工业中,安全壳内观检查能够直观地反映出安全壳性能,是非常重要的一项工作。现阶段,内观检查中的安全壳内衬鼓包测量主要采取人工测量的方式进行,针对传统方法效率低等问题,本文研制出一套新型的鼓包测量系统。该系统基于树莓派平台,采用激光位移传感器和超声波测距传感器,实现了安全壳鼓包的自动测量及自动识别功能,提高了工作效率,降低了工作成本。此外,设计试验对本系统进行精度分析,实例表明本系统测量精度优于内观检查精度要求,具有实用性和可行性。  相似文献   

准噶尔盆地车排子地区地层水离子参数特征与油气藏的关系     

占庆  郑庆伟  潘保芝 《世界地质》2015,34(2):524-530

准噶尔盆地车排子地区侏罗系与白垩系地层水矿化度整体较低,以Na HCO3水型为主。根据地层水化学成分特征,计算出多种离子比例系数,分析其与油气聚集的关系。研究表明:离子比例系数有明显的南北分区特征,南部凸起边缘封闭性不好,北部古隆起位于构造高部位,封闭条件较好,南部邻区四棵树凹陷的油气经南部断裂等输导体系运移到北部成藏。侏罗系地层水曾经遭受过比较强烈的大气降水的入渗,使早期油发生水洗氧化作用,形成现今大量的稠油油藏。侏罗系地层水封闭性好于白垩系,更有利于油气聚集和保存。  相似文献   

砂岩储层中碳酸盐胶结物定量识别及对含油性影响——以准噶尔盆地车北地区新近系沙湾组为例     

温雅茹  杨少春  赵晓东  向奎  朱春艳 《地质论评》2015,61(5):1099-1106

准噶尔盆地车排子地区北部新近系沙湾组砂岩储层中发育碳酸盐胶结物,该胶结物含量直接影响储层的含油性。为了定量识别碳酸盐胶结物,本文以岩芯常规分析数据为基础,利用图像分析软件进行微观薄片定量测量,弥补了岩芯常规分析数据的不足,发现车排子地区北部沙湾组砂岩中碳酸盐胶结物的含量(Y)与地层水中Ca~(2+)浓度(X)呈很好的正相关性(Y=0.0512·X~(0.7155)),相关系数达到0.93。利用地层水Ca~(2+)的浓度定量计算碳酸盐胶结物获得比较好的结果,解决了无实验分析井的碳酸盐胶结物含量求取的难题。对比分析碳酸盐胶结物数据和试油试采数据,发现碳酸盐胶结物含量≥20%的井基本不产油,碳酸盐胶结物含量20%的井产油性较好,表明碳酸盐胶结物控制车排子地区北部新近系沙湾组砂岩储层的含油性。  相似文献   

Harmonizing the RR Lyrae and clump distance scales – stretching the short distance scale to intermediate ranges?     

Piotr Popowski 《Monthly notices of the Royal Astronomical Society》2001,321(3):502-506

I explore the consequences of making the RR Lyrae and clump giant distance scales consistent in the solar neighbourhood, Galactic bulge and Large Magellanic Cloud (LMC). I employ two major assumptions: (i) that the absolute magnitude–metallicity, M _V (RR)–[Fe/H], relation for RR Lyrae stars is universal, and (ii) that absolute I magnitudes of clump giants, M _I (RC), in Baade's Window are known (e.g. can be inferred from the local Hipparcos -based calibration or theoretical modelling). A comparison between the solar neighbourhood and Baade's Window sets M _V (RR) at [Fe/H]=−1.6 in the range (0.59±0.05, 0.70±0.05), somewhat brighter than the statistical parallax solution. More luminous RR Lyrae stars imply younger globular clusters, which would be in better agreement with the conclusions from the currently favoured stellar evolution and cosmological models. A comparison between Baade's Window and the LMC sets M ^LMC(RC) _I in the range (−0.33±0.09,−0.53±0.09). The distance modulus to the LMC is μ ^LMC∈(18.24±0.08,18.44±0.07). Unlike M ^LMC(RC) _I , this range in μ ^LMC does not depend on the adopted value of the dereddened LMC clump magnitude, I ^LMC(RC)₀. I argue that the currently available information is insufficient to select the correct distance scale with high confidence.  相似文献   

The evolution from visible to infrared variable AGB stars     

J. A. D. L. Blommaert  R. Szczerba 《Astrophysics and Space Science》1994,217(1-2):143-144

Results of the Vassiliadis and Wood (1993) model for the evolution on the AGB are used to study how DENIS can complement an optical and IRAS based study of Long Period Variable AGB stars in a field towards the galactic bulge.  相似文献   

银河核球X射线源GX9＋1的振荡现象     

余文飞  季惕碚  程凌翔  孙学军  吴枚 《中国天文和天体物理学报》1994,(3)

分析１９８５年ＥＸＯＳＡＴ卫星对银河核球Ｘ射线源ＧＸ９＋１的观测数据，发现该源存在几百秒量级的振荡现象，这一结果有助于了解小质量Ｘ射线双星Ｇｘ９＋１的吸积特性和轨道运动。  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