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The abundances of 19 chemical elements in the atmospheres of five stars belonging to three globular clusters have been determined by applying the model-atmospheremethod to 430.0–790.0 nm spectra obtained with the échelle spectrometer of the 6-m telescope of the Special Astrophysical Observatory. The abundances of silicon, calcium, iron-peak elements, copper, zinc, and neutron-capture elements follow the abundance patterns for halo stars. The abundance of sodium in M 10 giants provides evidence that different mixing mechanisms operate in halo and cluster stars or that light elements are enriched in different ways in the pre-stellar matter from which some globular clusters and halo stars were formed. 相似文献
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Z. I. Peikov 《Astronomy Reports》2002,46(5):352-359
Lower limits for the percentages of stars with various luminosities in the cores of six globular clusters are derived using stellar spatial density distributions f(r) to deep limiting B magnitudes obtained earlier. For NGC 6535 and NGC 5466, the logarithmic density range and Kholopov parameters Df and Dr are also determined. These two parameters are correlated with the mean masses of stars of various subsystems and the total mass (number) of stars in the cluster. 相似文献
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Synthetic orthopyroxenes free of trivalent cations Mg x Fe 2-x Si2O6 (x=0; 1; 1.6) were investigated using both Mössbauer spectroscopy (MS) and single-crystal X-ray diffraction (XRD) in order to compare the results obtained on the same samples by the two techniques. The Mg-Fe distribution over M1 and M2 octahedral sites was determined on compounds with x = 1 and x=1.6, unheated and annealed at 650, 850 and 1040° C for 29 to 42 hours to obtain different degrees of order. The data obtained by the two techniques are in very good agreement, thus suggesting, for these compositions, the absence of systematic errors. The investigation of a synthetic compound with x=0 (ferrosilite) confirmed that the accuracy of both methods is very good. The observed small discrepancies between the results are not significant if compared with the relevant standard deviations which, for both methods, were derived by leastsquares calculations. The best fit is obtained for Fe(M1)/ Fe(tot) parameters that, in both methods, are directly calculated without using data from chemical analysis. For the unheated samples the values by MS and XRD are respectively: 0.185(9) and 0.180(4) for x = 1.6; 0.282(8) and 0.285(2) for x=1; 0.503(7) and 0.502(1) for x=0. For all the investigated samples the correlation between the geometrical distortion parameters, calculated by X-ray refinement, and the quadrupole splitting values, measured by Mössbauer spectroscopy, agrees with the theoretical model of Ingalls (1964). 相似文献
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The geographic backdrop of the work of three noted South American writers is reviewed under the stylistic categories of tellurism, mythical realism and magical realism. The acute sense of place demonstrated by these authors is explained on the basis of ethnical roots, collective mental constructs and colonial experiences. José María Arguedas has offered a poignant socio-mythical interpretation of the rise and fall of Chimbote, Peru's major fishing port in his postumous novel El zorro de arriba y el zorro de abajo which is useful to grasp the problems of that country. The atmosphere of Caribbean Colombia has been recorded with great vigor in several novels of Gabriel García Márquez. Tellurism acquires a particular significance in three poems of Neruda which are presented as examples of his poetic views of physical Chilean landscapes and the select use of vocables. 相似文献
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为深化潟湖相碳酸盐岩储集层非均质性认识,以伊拉克M油田白垩系Mishrif组为例,基于岩心观察、物性分析数据、铸体薄片及压汞实验,对潟湖相储集层特征及成因机理开展研究.结果显示:研究区潟湖环境岩石类型复杂,生物碎屑具有多样性,储集层以低渗、特低渗为主,孔隙度分布范围宽,发育大量的基质微孔、铸模孔和晶间孔.储集层强非均质性是复杂沉积作用和差异成岩作用的结果.潟湖沉积物泥质含量高,发育大量基质微孔,与生物扰动作用相伴生的埋藏白云化作用可形成晶间孔,易溶型生物碎屑被选择性溶蚀形成大量的铸模孔.研究认为:潟湖沉积物原始物性较低,后期成岩作用可改善储集层物性.生物扰动期次、扰动强度、充填物类型、环境的封闭性及外来流体性质等因素控制了潜穴中充填物的改造趋势;生屑类型、成岩序列和成岩环境等影响了沉积物中铸模孔的发育和保存.综合潜穴充填物类型、生屑类型、成岩环境和成岩作用等因素,建立了生物扰动成因孔隙模式和铸模孔发育模式. 相似文献
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Mineralium Deposita - 相似文献
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大别山是中国东部中朝大陆板块与扬子大陆板块之间的碰撞造山带。具有薄皮构造的性质。组成两个碰撞大陆之间的滑脱（冲断剪切）带的岩石就是碰撞混杂岩组合。大别山由于剥露较深,仰冲壳楔完全被剥蚀,超高压变质带大面积出露,识别出碰撞混杂岩组合是对大别山进行几何分析的必要步骤。大别山碰撞混杂岩组合可分为南北两部分。北部为条带状片麻岩-超镁铁岩组合,南部为云母斜长片麻岩-榴辉岩组合,这两个组合的大部分都经历过超高压变质作用。它们的共同特点是具有宏观的＂碎斑结构＂和混杂作用。罗田穹隆是造山过程中早期形成的双冲式背斜,最后在造山晚期因东西向缩短的叠加而形成穹隆。 相似文献