CCD‐Δa and BV R photometry of NGC 7296

The first CCD photometric investigation of the open cluster NGC 7296 up to now was performed within the narrow band Δa photometric system, which enables us to detect peculiar objects. A deeper investigation of that cluster followed, using the standard BV R ‐Bessel filter set. The age and E (B – V ) was determined independently to log t = 8.0 ± 0.1 and 0.15 ± 0.02, respectively by using Δa and broadband photometry. In total five Be/Ae objects and two metal‐weak stars showing significant negative Δa ‐values as well as one classical chemically peculiar star could be identified within that intermediate age open cluster. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Magnetic fields in massive star-forming regions

We present the largest sample of high-mass star-forming regions observed using submillimetre imaging polarimetry. The data were taken using the Submillimetre Common User Bolometer Array (SCUBA) in conjunction with the polarimeter on the James Clerk Maxwell Telescope (JCMT) in Hawaii. In total, 16 star-forming regions were observed, although some of these contain multiple cores. The polarimetry implies a variety of magnetic field morphologies, with some very ordered fields. We see a decrease in polarization percentage for seven of the cores. The magnetic field strengths estimated for 14 of the cores, using the corrected Chandrasekhar and Fermi (CF) method, range from <0.1 mG to almost 6 mG. These magnetic fields are weaker on these large scales when compared to previous Zeeman measurements from maser emission, implying the role of the magnetic field in star formation increases in importance on smaller scales. Analysis of the alignment of the mean field direction and the outflow directions reveals no relation for the whole sample, although direct comparison of the polarimetry maps suggests good alignment (to at least one outflow direction per source) in seven out of the 15 sources with outflows.     

Fundamental parameters and new variables of the galactic open cluster NGC 7128

CCD photometry in Johnson UBV and Strömgren uvby systems and medium-resolution spectroscopy of the galactic open cluster NGC 7128 are presented. Spectral types of the brightest 12 stars in the cluster field were determined based on equivalent widths of the H α and the He  i 6678-Å line. The spectroscopic observations also revealed two obvious and one probable Be-type stars showing H α emission. The analysis of the photometric diagrams gave a colour excess of E ( B − V )=1.03±0.06 mag, a distance modulus DM =13.0±0.2 mag and an age above 10 Myr. Time-resolved photometric observations obtained on one night resulted in the detection of short time-scale light variations of seven new and three already known variable stars in the cluster field.     

Wavelet domain Bayesian denoising of string signal in the cosmic microwave background

An algorithm is proposed for denoising the signal induced by cosmic strings in the cosmic microwave background. A Bayesian approach is taken, based on modelling the string signal in the wavelet domain with generalized Gaussian distributions. Good performance of the algorithm is demonstrated by simulated experiments at arcminute resolution under noise conditions including primary and secondary cosmic microwave background anisotropies, as well as instrumental noise.     

A Reinvestigation of the Physical Properties of Pismis 3 based on 2MASS Photometry

As a continuation of a series of work, we aim to refine and re-determine the physical parameters of previously rarely or un-studied open star clusters with good quality CMDs using Near-IR JHK photometry. Here we present a morphological analysis of the 2MASS database (the digital "Two Micron All Sky Survey") for the open cluster Pismis 3. Some of the physical parameters are estimated for the first time, and some others, re-determined.     

城市雨洪模拟技术研究进展

从对水文过程描述的角度对城市雨洪模拟技术进行了回顾,认为管网汇流阶段算法较为成熟,而产流和坡面汇流阶段还有待深入研究.从模型构建思想的角度回顾其发展历程,阐明了经验性模型和分布式概念性模型的局限性以及分布式物理模型的良好发展前景.通过总结国内外几个具代表性城市雨洪模型的特点,从特定模型的角度进一步分析城市雨洪模型的现状,并指出中国与国外模型研究的差距.对与城市雨洪模拟精度密切相关的基础数据收集与管理技术进行了讨论,并提出了城市雨洪模拟技术的发展方向.     

渤中25-1油田沙河街组低孔低渗储层特征及分类评价

渤中25-1油田位于渤海南部海域,其主力油层为古近系沙河街组,总体上属于低孔低渗储层。通过薄片、扫描电镜、X衍射分析和测井解释等手段,对沙河街组砂岩储层的岩石学特征、沉积特征、物性和孔隙结构特征进行了分析研究。沙河街组沙三段为较深水湖泊环境下的浊积扇沉积,沙二段为扇三角洲沉积;岩性主要为岩屑长石砂岩,储层孔隙类型为混合孔隙、次生孔隙和原生孔隙,由于沙三段溶蚀孔隙发育较沙二段少,沙三段物性较沙二段差。结合储层试油结果,提出了低孔低渗储层宏观成因、微观孔隙结构和综合评价3种分类方案,总体上把储层分为好、中和差3类,对应产能分别为大于80 m3/d、介于10~100 m3/d之间、小于10 m3/d和微量或无产能。经过该油田沙河街组5口井、15个储层段的测试验证,储层宏观成因分类评价结果与实际试油结果符合率达到86.67%,微观孔隙结构分类和综合分类评价结果与实际试油结果基本吻合。     

清江水布垭水利枢纽地下厂房围岩变形特性研究

通过在水布垭水利枢纽地下厂房中进行变形试验,研究了厂房区岩体的变形特性,采用反分析法进行粘弹性反分析,反演出地应力、弹性模量及粘性参数,并与现场试验结果进行比较,对反算值进行评价。     

BOOK REVIEWS

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