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为探讨大别造山带早期结晶基底物质组成及其演化特征,对大别造山带蕙兰山地区出露的黑云紫苏斜长片麻岩的岩石学、地球化学、锆石U-Pb年代学及Lu-Hf同位素组成进行研究,显示其原岩应为石英闪长岩,成岩时代为古元古代早期(2463±22 Ma),且经历了古元古代麻粒岩相变质作用,锆石Ti地质温度计显示其变质温度为767~827℃(平均799℃),变质时间为2002±11 Ma(MSWD=0.46)。岩石地球化学成分显示其SiO2含量为55.16%~57.10%,MgO为4.74%~5.89%,Mg#值为47.5~50.4,钙碱性系列,富Mg贫Si,稀土配分曲线呈现轻稀土相对富集的右倾分布特征((La/Yb)N=19.3~34.1),无明显Eu异常((Eu/Eu*)=0.9~1.2),且具较高的Sr、Ni、Cr含量,以及较低的YbN值及Y含量,与镁质闪长岩具相似特征;明显富集Rb、Ba、K等大离子亲石元素,相对亏损Nb、Ta、Zr、Hf等高场强元素;锆石Lu-Hf同位素显示具有较为均一... 相似文献
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通过利用CANDELS-EGS(Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey-Extended Groth Strip)场中HST WFC3(Hubble Space Telescope Wide Field Camera 3)F160W高分辨率的观测图像,研究了9个光谱红极亮红外星系的形态结构特征.发现这些星系的形态表现出多样性(从椭圆到多个亮核或弥散的结构),如:双核,气体桥,双不对称体,不规则或椭圆结构.为了定量地研究这些极亮红外星系的形态,测量了它们在静止光学波段的形态参数(基尼系数G和矩指数M20).与近邻极亮红外星系相比,高红移极亮红外星系的G偏小而M20偏大,表明这些星系的星族分布聚集度小且不对称性大.基于对样本中极亮红外星系2维面亮度轮廓的拟合,得到这些星系的有效半径分布在2.4 kpc到5.8 kpc之间,其平均值是(3.9±1.1)kpc.相比较于近邻相似质量的恒星形成星系来说,高红移极亮红外星系的平均大小要小1到2倍.在类似红移和红外光度条件下,得出的这些结果也与其它文献中给出的结论相一致. 相似文献
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KONG Xu LIN Lin LI Jin-rong ZHOU Xu ZOU Hu LI Hong-yu CHEN Fu-zhen DU Wei FAN Zhou MAO Ye-wei WANG Jing ZHU Yi-nan ZHOU Zhi-min 《Chinese Astronomy and Astrophysics》2014
In recent years the number of worldwide 8∼10 m-class ground-based telescopes is continually increased, the 4 m-diameter or smaller telescopes have become the small and medium-sized telescopes. In order to obtain some noticeable scientific results by using these existing small and medium-sized telescopes, we have to consider very carefully what we can do, and what we can not. For this reason, the Time Allocation Committee of the 2.16 m telescope of the National Astronomical observatories of China (NAOC) has decided to support some key projects since 2013. The long-term project “Spectroscopic Observations of the Star Formation Regions in Nearby Galaxies” proposed by us is one of three key projects, it is supported by the committee with 30 dark/grey nights in each of three years. 相似文献
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An analysis of a selection experiment was used to assess the impact of various animal model structures on REML estimates of variance components.The analyses were carried out based on 162 d body mass (BM) of 1 287 animals from 21 paternal half-sib groups of Fenneropenaeus chinensis.Estimated breeding values (EBV) of BM of all individuals were estimated using eight statistical models (A,AB,ABC,ABDC,ABMFC,ABMDC,ABFDC and ABMFDC) and BLUP (best linear unbiased prediction).These models were designed involving factors such as sex,spawn date as fixed effects,maternal genetic effects,full-sib family effects as random effects,mean BM of families at tagging and age at recording (covariate).The results demonstrate the importance of correct interpretation of effects in the data set,particularly those that can influence resemblance between relatives.The data structure and the particular model that was applied markedly influenced the magnitude of variance component estimates.Models based on few effects obtained upward biased estimates of additive genetic variance.The accuracy of genetic parameters and breeding value estimated by ABFDC model was higher than other models.The results imply that additive genetic direct value,full-sib family effects,and covariance effects besides sex and spawn date as fixed effects were very important for estimating genetic parameters and breeding value of body mass.This model had a heritability estimate of 162 d BM of 0.44.The comparison of the efficiency of selection based on breeding values or phenotypic value revealed great difference:average breeding value of the best 24 families selected by the 162 d BM breeding value and phenotype were 0.577 g and 0.366 g,respectively,representing a 36.57% higher efficiency in the former.In conclusion,selection based on breeding value was more effective than selection based on phenotypic value.Our results indicate that effects influencing the magnitude of estimates should be taken into account when estimating heritability and breeding values for BM. 相似文献