The Yields of r-Process Elements and Chemical Evolution of the Galaxy

The supernova yields of r-process elements are obtained as a function of the mass of their progenitor stars from the abundance patterns of extremely metal-poor stars on the left-side [{Ba/Mg}]--[{Mg/H}] boundary with a procedure proposed by Tsujimoto and Shigeyama. The ejected masses of r-process elements associated with stars of progenitor mass M _ms ≤ 18 M _⊙ are infertile sources and the SNe II with 20 M _⊙ ≤ M _ms ≤ 40 M _⊙ are the dominant source of r-process nucleosynthesis in the Galaxy. The ratio of these stars 20 M _⊙ ≤ M _ms ≤ 40 M _⊙ with compared to the all massive stars is about∼ 18%. In this paper, we present a simple model that describes a star's [r/Fe] in terms of the nucleosynthesis yields of r-process elements and the number of SN II explosions. Combined the r-process yields obtained by our procedure with the scatter model of the Galactic halo, the observed abundance patterns of the metal-poor stars can be well reproduced.     

观测结果对三成分多分量星系化学演化模型的约束

本文是在银河系化学演化的基础上,利用银河系的三成分(threezone)(即晕、厚盘和薄盘)多相(multi phase)(气体,分子云,大、小质量恒星以及剩余物质)的化学演化的理论模型,讨论了以下观测约束:1、质量面密度、恒星形成率,各分区质量比;2、场星的年龄-金属丰度关系;3、α元素化学演化;4、太阳附近G矮星金属丰度分布;5、三成分金属丰度特征量;6、超新星爆发率;7、内落速率。结果表明,三成分多分量模型能够较好地满足观测约束,比较真实地反映星系演化过程。可以用该模型计算元素的星系化学演化。     

Chemical Evolution of Blue Compact Galaxies

Based on a sample of 72 Blue Compact Galaxies (BCGs) observed with the 2.16m telescope of the National Astronomical Observatories, Chinese Academy of Sciences (NAOC) and about 4000 strong emission line galaxies from the Sloan Digital Sky Survey, we analyzed their chemical evolution history using the revised chemical evolution model of Larsen et al. Our sample covers a much larger metallicity range (7.2 < 12 log(O/H) < 9.0). We found that, in order to reproduce the observed abundance pattern and gas fraction over the whole metallicity range, a relatively continuous star formation history is needed for high metallicity galaxies, while assuming a series of instantaneous bursts with long quiescent periods (some Gyrs) for low metallicity galaxies. Model calculations also show that only the closed-box model is capable of reproducing the observational data over the whole metallicity range. Models that consider the ordinary winds and/or inflow can only fit the observations in the low metallicity range, and a model with enriched wind cannot fit the data in the whole metallicity range. This implies that the current adopted simple wind and inflow models are not applicable to massive galaxies, where the underlying physics of galactic winds or inflow could be more complicated.     

Abundance and Biomass of Benthic Bacteria in Jiaozhou Bay, China

The abundance and biomass of benthic heterotrophic bacteria were investigated for the 4 typical sampling stations in the northern muddy part of Jiaozhou Bay, estuary of the Dagu River, raft culturing and nearby areas of Huangdao in March, June, August and December, 2002. The abundance and biomass range from 0.98×10⁷ to 16.87×10⁷ cells g⁻¹ sediment and 0.45 to 7.08 μg C g⁻¹ sediment, respectively. Correlation analysis showed that heterotrophic bacterial abundance and biomass are significantly correlated to water temperature (R=0.79 and 0.83, respectively,P<0.01).     

Comparative analysis on utilisation of linear spectral unmixing and band ratio methods for processing ASTER data to delineate bauxite over a part of Chotonagpur plateau,Jharkhand, India

We have attempted comparative analysis of the utility of linear spectral unmixing (LSU) method and band ratios for delineating bauxite from laterite within the lateritic bauxite provinces of Chotonagpur Plateau, Jharkhand of India. This was attempted based on processing of visible–near infrared (VNIR) and shortwave infrared (SWIR) spectral bands of Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) sensor. In LSU method, spectral features of main constituent minerals of lateritic bauxite are used to decompose the pixel spectra to estimate the relative abundance of bauxite and laterite in each pixel to spatially delineate bauxite within laterite. We have also compared the bauxite map derived using LSU method with bauxite maps of two band ratios in terms of spatial disposition of bauxite. We also have attempted to relate the abundance values of pixels of LSU-based bauxite map with band ratio values of bauxite pixels of two selected bauxite indices.     

手性污染物六溴环十二烷在食物链传递中的选择性及生物放大作用研究进展

六溴环十二烷(HBCDs)是一种全球生产的添加型溴化阻燃剂,被广泛应用于隔热建筑材料阻燃剂、室内装潢、纺织品和电子产品中,不仅对生态环境造成污染,而且还会通过食物链的传递危害人类健康。研究生态系统中HBCDs异构体及对映体的环境行为与生物放大作用是进行环境风险评估和有效控制污染的生态学基础。基于此,本文从HBCDs的基本特性出发,阐述了HBCDs异构体及对映体在食物链中的选择性生物富集放大及转化行为,分析了发生选择性富集及转化的影响因素,这些因素包括生物体的生活环境、饮食习惯、所处食物链中营养级水平以及HBCDs选择性吸收、代谢和异构化等。已有的研究报道显示HBCDs异构体及对映体在生态系统中的富集、转化及生物放大行为不是单一的过程,是生物体和环境多因素综合的结果。今后应对HBCDs异构体及对映体在各种食物链(如淡水食物链和陆生食物链)中的选择性环境行为以及在食物链传递中发生选择性的主控因素等方面进行深入系统的研究,为全面评价其生态风险提供科学依据。     

海洋石油降解菌群的固定化及石油降解特性

为克服岸滩溢油生物修复过程中海浪冲刷等不利环境对石油降解菌(群)岸滩定植的影响,本文利用聚乙烯醇(PVA)和海藻酸钠作为载体对石油降解菌群DC10进行固定化,通过研究细菌固定化微球的机械性能、传质性能及石油降解特性等参数,确定石油降解菌群的最优固定化条件。实验结果表明:6%PVA,2%海藻酸钠及0.5%活性炭制备的凝胶可以通过蠕动泵方便快捷制备细菌固定化微球,其粘度小、易成型、机械强度高。海洋石油降解分析表明,与游离菌体(FB)相比,固定化菌群12d石油降解率提高了近7%;GC-MS分析显示,石油烷烃和芳烃降解效果显著。实验证明,石油降解菌群DC10经过固定化处理,其石油降解活性提高,连续降解能力增强,该研究为溢油岸滩的生物修复提供新的技术方法。     

基于NDVI与丰度关系的MODIS影像浒苔混合像元分解方法

MODIS影像是浒苔业务化卫星遥感监测的重要数据源,但其空间分辨率(250m)较低,混合像元效应导致传统的NDVI(Normalized Difference Vegetation Index)阈值法浒苔提取误差较大。为解决此问题,本文以准同步的较高分辨率的HJ-1CCD影像浒苔提取结果为基准,建立基于MODIS NDVI与浒苔像元丰度(浒苔覆盖面积占像元面积百分比)关系的浒苔信息提取模型,利用该模型可提取每个像元的丰度(即浒苔覆盖率),从而提高整景影像浒苔覆盖面积提取精度。该模型可为浒苔灾害等级的确定以及防灾减灾应急决策提供支持。     

内蒙古林西地区上二叠统林西组烃源岩有机岩石学特征

内蒙古东部林西地区是二连盆地外围石炭-二叠系油气勘探的重要潜力区之一．为了研究上二叠统林西组烃源岩有机岩石学特征,对野外露头剖面的林西组烃源岩开展了总有机碳、有机显微组分、镜质体反射率及岩石热解等测试分析.结果表明：林西组烃源岩总有机碳分布在0.63%～1.30%,平均为0.87%,所有样品含量均大于0.6%;有机显微组分分布在0.27%～3.66%,平均值为2.08%,其中95.24%的样品达到1.0%以上,表明有机质丰度达到了“较好”至“好”级别;镜质体反射率分布在1.26%～2.58%,平均值为1.88%,其中90.47%的样品含量大于1.3%,镜质体反射率较高,表明有机质成熟度达到“高成熟”至“过成熟”阶段;岩石热解氢指数分布在8×10-3～89×10^-3,平均为27.52×10^-3,表明有机质类型归属于Ⅲ型.综合评价表明林西地区上二叠统林西组烃源岩属于“较好—好”烃源岩,生烃潜力较大,具有较好的油气资源前景.