类星体Lyα吸收线密度与其发射线红移的关系

本文利用７２个具有中等分辨率的类星体Ｌｙα线资料，研究了Ｌｙα吸收线数密度Ｎ（Ｚａｂｓ）与类星体发射红移Ｚｅｍ的变化关系，结果表明：对于Ｚｅｍ越大的类星体其全部Ｌｙα吸收线的平均数密度Ｎ（Ｚａｂｓ）也越大，但对于相同的吸收红移值而言，Ｎ（Ｚａｂｓ）在统计意义上与Ｚｅｍ并无关系。本文还将所得结果与其他的有关工作作了比较及讨论。     

吉林东柳河子矿区找矿突破探讨

我国正处于工业化、城镇化,加快推进和全面建设小康社会的关键时期。面对我国经济长期持续较快发展,矿产资源消费加速,供需矛盾日益突出。本文以吉林省辽源市椅山-东柳河子矿区找矿突破的实践为例,探索区域矿产资源勘查开发新理论、新机制、新实践,努力做到找矿目标明确、与时俱进,深入综合分析、提高找矿能力,开发新机制,加速推进找矿突破的新实践,努力实现矿产资源的可持续利用、促进经济社会可持续发展的战略目标。     

蟠龙山红旗漫卷硝烟弥漫 盘龙寨军旗招展战火熊燃 狮子寨旌旗飘遍战斗正酣 黄猫垭以红四方面军战胜敌军“六路围攻”策应中央红军北上抗日巨大胜利使其地名释放光彩

黄猫垭位于四川省苍溪县城东北102公里的蟠龙山梁上,山上盘龙寨和狮子寨之间的岩壁上,有一对黄色巨石其形若猫,故名黄猫垭。位于旺苍与苍溪交界处的黄猫垭,四周山峦起伏,悬崖挺立,十分险要,是木门场通往苍溪的咽喉。当年,红四方面军     

滇东石漠化伴生“红裸土”表层有机质含量与酸碱度关系分析

对滇东地区石漠化伴生"红裸土"典型发育地带的表层样品的有机质和酸碱度分析表明:"红裸土"表层有机质含量范围为0.60～38.5(g.kg-1),平均值为13.49(g.kg-1);酸碱度在4.20～5.72。不但"红裸土"表层有机质含量低,呈中强酸性,且"红裸土"表层土壤有机质含量与酸碱度成弱正相关。这一特征与同区域有植被覆盖下的表层土壤相反,与其他典型的喀斯特地区土壤表层有相似的变化规律。这些特征说明"红裸土"可能是形成石漠化过程的一个阶段。     

星系的红移

红移（redshift）对于天文爱好者来说是一个非常熟悉的概念了。根据多普勒效应,波源朝向观察者运动时,光谱会向短波端移动,叫做紫移（blueshift）;反之,当波源背向观察者运动时,光谱就会移向长波端,产生红移（redshift）。     

Growth of Black Holes and Their Host Spheroids in （Sub）mm-loud High-Redshift QSOs

We study the growth of black holes and stellar population in spheroids at high redshift using several （sub）mm-loud QSO samples. Applying the same criteria established in an earlier work, we find that, similar to IR QSOs at low redshift, the far-infrared emission of these （sub）mm-loud QSOs mainly originates from dust heated by starbursts. By combining low-z IR QSOs and high-z （sub）mm-loud QSOs, we find a trend that the star formation rate （M＊） increases with the accretion rate （Mace）. We compare the values of M＊/Macc for submm emitting galaxies （SMGs）, far-infrared ultraluminous/hypeduminous QSOs and typical QSOs, and construct a likely evolution scenario for these objects. The （sub）mm-loud QSO transition phase has both high Macc and M＊ and hence is important for establishing the correlation between the masses of black holes and spheroids.     

A GRB Follow-up System at the Xinglong Observatory and Detection of the High-Redshift GRB 060927

A gamma-ray burst (GRB) optical photometric follow-up system at the Xinglong Observatory of National Astronomical Observatories of China (NAOC) has been constructed. It uses the 0.8-m Tsinghua-NAOC Telescope (TNT) and the 1-m EST telescope, and can au-tomatically respond to GRB Coordinates Network (GCN) alerts. Both telescopes slew rela-tively fast, being able to point to a new target field within ～ 1 min upon a request. Whenever available, the 2.16-m NAOC telescope is also used. In 2006 the system responded to 15 GRBs and detected seven early afterglows. In 2007 six GRBs have been detected among 18 follow-up observations. TNT observations of the second most distant GRB 060927 (z = 5.5) are shown, which started as early as 91 s after the GRB trigger. The afterglow was detected in the combined image of the first 19 × 20 s unfiltered exposures. This GRB follow-up system has joined the East-Asia GRB Follow-up Observation Network (EAFON).     

新疆阿尔泰山南缘红墩SEDEX型铅锌矿的成矿模式

克兰裂谷盆地位于新疆阿尔泰山南缘的中部,其沉积构造演化经历了三个阶段：早期酸性火山-沉积阶段;中期基性火山-沉积阶段;晚期碎屑沉积阶段。红墩铅锌矿床形成于盆地中期基性火山-沉积阶段的被动陆缘裂谷构造环境,具有SEDEX型铅锌矿床的地质特征,找矿潜力大。