Contact Binaries: A Study of the Proximity Effects and Gravity Darkening Based on Kopal’s Fourier Method

A new method for the determination of the proximity effects and gravity darkening exponents in contact binaries of W UMa type is presented. The method is based on Kopal’s method of Fourier analysis of the light changes of eclipsing variables in the Frequency Domain. The method was applied to 36 W UMa systems for which geometric and photometric elements have been derived by the most powerful techniques. The derived values are very close to those predicted by the existing theory of radiative transfer or convective equilibrium.     

V2213 Cyg is a New W Uma-Type System

V2213 Cyg was discovered as a variable star by Pavlenko (1999) in 1998. We present our photometry of V2213 Cyg from 1998–2003 based on CCD observations with the K-380 Cassegrain telescope of CrAO and the 60 cm Zeiss telescope of SAI. Observations have been carried out mostly in R and sometimes in B and V Johnson system. The total amount of data is 2270 points, covering ∼50 nights. We classify this binary as a W UMa-type contact system. Using all data we determined the orbital period to be 0.350079 ± 0.000007 day. The mean brightness varies between R = 14.35 and 14.05. The mean 1999–2003 orbital light curve has two humps and a primary minimum (I), which is 0.04 mag brighter than the deeper secondary one (II). The mean humps have slightly different height. The difference between two individual maxima varies within 0.1 mag, which may indicate an activity of the components. The highest hump is an asymmetrical one: it has sort of a shoulder at phases 0.75–0.80, before entering the less deep primary minimum (phase 0.0). The system is rather reddened, its colour indices are: B−V ∼ 0.8 and V−R ∼ 0.7, and give a spectral class of V2213 Cyg earlier than K.     

Photometric Study Of W Uma Type Binary In The Old Cluster Ngc 6791

Study of eclipsing binaries in an open cluster offer information regarding the age of the cluster in addition to the component stars. In this paper we present the analysis of a W UMa system discovered in the open cluster NGC 6791 using the Wilson–Devinney (W–D) method.     

黑龙江双鸭山地区白钨矿勘查开发的思考

双鸭山铁矿早已被开发利用,而钨矿却被忽略。文章通过对该成矿区典型矿床的地质特征,矿物学特征研究认为,铁矿、钨矿往往处于同一成矿区段,相伴产出,因此在该地区应加强钨矿的勘查力度。在矿床开发方面应统一布局,合理开发利用,达到资源利用最大化。     

南秦岭构造带内早古生代碱基性岩浆活动：古特提斯洋裂解的证据

位于南秦岭构造带南缘的勉略(勉县—略阳)洋是东古特提斯洋的北侧分支洋盆,在勉县—略阳地区发育有典型的蛇绿岩组合。然而,由于中三叠世晚期开始的碰撞造山作用以及之后陆内变形作用的改造,对于勉略洋盆在构造带东段的裂解和演化过程并不清晰。本文对发育于东南秦岭构造带内的基性岩墙群进行了岩石学、岩石地球化学、同位素年代学等方面的研究。结果表明,基性岩脉以辉长岩、辉绿岩等基性岩为主,其SiO 2含量为41.89%~49.75%,属基性—超基性岩类,并具有富钠、高钛的碱性岩特征。岩石的稀土、微量元素和Sr—Nd同位素特征与板内洋岛玄武岩(OIB)特征一致,岩浆源于具有地壳混染的板内洋岛玄武岩型地幔源区。该类基性岩脉顺层侵入到早古生代早期地层中,通过基性岩脉中的锆石SHRIMP测年获得岩脉顺层侵位的时代为晚志留世早期(约422 Ma)。这种岩浆作用很可能与古特提斯洋初始裂解有关,并导致南秦岭构造带内地壳伸展、基性岩浆侵位,该过程与南秦岭构造带北缘的商丹(商南—丹凤)原特提斯洋的消减和陆内俯冲可能相关。     

西藏首例云英岩型钨矿——甲岗雪山W-Mo多金属矿床地质特征研究

甲岗雪山W-Mo多金属矿床位于西藏自治区申扎县境内,地处冈底斯北部,成矿时代为中新世。矿床与矿区内的二长花岗岩体时空关系紧密,矿区内的围岩蚀变普遍见云英岩化,并且云英岩化强烈的地方多伴随强烈的钨钼矿化;矿体的类型以云英岩型为主,还有少量石英脉型,矿石又多呈细脉状或浸染状赋存于云英岩或云英岩化二长花岗岩体内部,证实了矿床的成因类型为云英岩型。依据野外见到的矿物共生组合、脉体穿切关系等,可将成矿期划分为硅酸盐-氧化物阶段和硫化物阶段。流体包裹体研究表明,甲岗雪山W-Mo多金属矿床主成矿期的成矿流体为中-高温、中-低盐度的流体,从主成矿期的硅酸盐-氧化物阶段演化到硫化物阶段,成矿流体的温度下降明显,盐度也有所下降。     

地球核幔相互作用的W同位素研究进展

地球核幔相互作用的研究难点在于无法获得实际样品。洋岛玄武岩和溢流玄武岩被认为是地幔柱减压熔融的产物,携带了核幔边界的物质信息,可作为研究地球核幔相互作用的样品。¹⁸²Hf-¹⁸²W同位素体系的特殊化学性质,使W同位素成为研究核幔相互作用的重要工具。本文介绍了W同位素示踪的基本原理,并回顾了核幔相互作用的W同位素研究进展。目前已发表的数据表明,全球洋岛玄武岩具有W元素丰度富集(67×10^-9~855×10^-9)、¹⁸²W同位素亏损(μ¹⁸²W=-0.1~-16.1)的特征,由此推断洋岛玄武岩可能来源于核幔平衡源区。Baffin Bay和Ontong Java Plateau溢流玄武岩则具有¹⁸²W富集(μ¹⁸²W=23.4)的特征,可能来源于早期地幔源区。洋岛玄武岩和溢流玄武岩的μ¹⁸²W差异可能是由地幔柱头尾异质性引起。此外,引起μ¹⁸²W异常的其他原因可能有：原始地幔源区的隔离保存、后增生薄层物质的部分混入和低效的核幔分异作用等。目前,W同位素的核幔交换机制仍不清楚。

     

青海省河南县三叠系伊利石结晶度与极低级变质作用

在开展“青海省河南县托叶玛地区I47E007023、I47E008023、I47E009023、1I47E009024四幅1:5万区域地质矿产调查”时,为验证该地区三叠系变质情况,针对三叠系中泥岩(页岩)的伊利石结晶度做了分析测试。30件样品的实验结果表明: 北部宗务隆—泽库地层分区三叠系泥岩(页岩)伊利石Kübler结晶度指数为0.312~0.537,晶胞参数b₀为0.898 0~0.903 2 nm,判断其变质温度小于350 ℃,具葡萄石-绿纤石和沸石相; 南部西倾山地层分区三叠系泥岩(页岩)的伊利石Kübler结晶度指数为0.21~0.318,b₀为0.898 1~0.901 4 nm,变质温度主要分布在200~350 ℃,局部>350 ℃,具葡萄石-绿纤石和绿片岩相。研究认为青海省河南县地区区域变质程度较低,为极低级变质作用或者未发生区域变质作用,且南部西倾山地层分区的变质程度略高于北部宗务隆—泽库地层分区变质程度。这一变质相带研究结论与前人认为的“区域低温动力变质作用及低绿片岩相变质带”不一致,变质程度相对更低。该研究证实了在青海省河南县地区三叠系地层中不存在大面积区域变质作用,仅存在极低级区域变质作用。     

西藏察隅县那阿钨床成矿地质特征与找矿前景

那阿钨矿为矽卡岩型白钨矿床,矿体产于沿北西向分布的二长花岗岩岩体与大理岩的外接触带的矽卡岩及其强矽卡岩化大理岩中,其规模、形态、产状严格受矽卡岩岩性控制,自南向北矿体埋藏深度逐渐加大,向深部钨矿化有变好趋势。围岩蚀变主要有矽卡岩化、硅化及碳酸岩化等。通过对矿区的成矿地质条件进行分析,总结分析了区内找矿及成矿标志,提出了有益建议。     

Holocene record of productivity in the NW Iberian continental shelf

A multiproxy approach (textural characteristics, heavy metal concentrations and benthic foraminifera data) was adopted to study the OMEX core KSGX 40, collected at the Galicia Mud Deposit (NW Iberian outer continental shelf) and recording the last ca. 4.8 ka cal BP. Geochemical profiles of Fe, Mn, Zn, Co, Cr, Cu, Ni, Pb, Al and Ca show significant temporal variations. Benthic foraminifera productivity proxy suggests that the recorded muddy events were contemporaneous of a higher C_org flux to the marine benthic environment. The higher flux of organic matter, following a long-term intensification of the upwelling and coinciding with a finer sedimentation, led to depressed levels of oxygen beneath the water-sediments interface and to early diagenetic processes of several redox-sensitive elements.