O-rich SR and Mira variables in DENIS     

J. Hron  F. Kerschbaum 《Astrophysics and Space Science》1994,216(1-2):137-138

Previous VLA observations of the triple radio continuum source in Serpens showed that it has very unusual and extraordinary characteristics. While this source is associated with a star forming region, its outer components exhibit a combination of thermal and nonthermal spectra and large proper motions, Furthermore, the NW lobe has knotty and extended emission connecting the central source with the bright outer knot. Here, we present results of new VLA radio continuum high-angular resolution observations of this Radio Jet. Combining these observations with those obtained previously, we find that: a) one of the knots along the main body of the radio jet (knot G) exhibits proper motions similar to those observed in the outer NW and SE components, and the time variable knot A; b) the outer knots are moving away from the central source in slightly different directions; and c) the orientation of the central source seems to change with time. These results are consistent with a central precessing source that undergoes periodic ejection of material.  相似文献   

西藏知不拉和浪母家果矽卡岩铜矿地质特征及驱龙-知不拉-浪母家果成矿系统的确定   总被引：1，自引：0，他引：1  

王登芳 《地质与勘探》2015,51(4):619-633

西藏驱龙巨型斑岩铜钼矿床周围产出有知不拉与浪母家果矽卡岩铜矿。通过揭示知不拉和浪母家果的地质特征、成矿侵入体的地球化学特征和硫同位素特征,结合前人的年代学资料,确立两者与驱龙斑岩铜矿共同构成斑岩-矽卡岩成矿系统。结果显示知不拉与浪母家果矽卡岩矿床中的侵入岩地球化学特征与驱龙矿区的侵入岩地球化学特征相似,属于准铝质、钙碱性-高钾钙碱性岩石;稀土元素表现为强烈的LREE和HREE的分异,除知不拉的细晶岩有很强的Eu负异常,其他具有很弱的Eu负异常;明显富集大离子亲石元素(LILE)和高场强元素(HFSE),K、Pb的正异常,Ta、Nb、Ti的负异常。知不拉硫化物硫同位素与驱龙斑岩铜钼矿的硫同位素相比有明显的差异,这样的差异可能是由于成矿热液氧逸度的变化和晚期高δ34S值的天水加入造成的。研究确立驱龙-知不拉-浪母家果斑岩-矽卡岩成矿系统,主要基于:时代相近,空间毗邻;驱龙斑岩铜矿花岗闪长岩接触带发育有明显矽卡岩矿化;与矿化有关的侵入岩地球化学特征相似性;成矿物质演化趋势相似;矽卡岩连续演化的物理化学条件。而钙质围岩、多期次侵位且侵位较浅的岩浆与区域内构造活动及矿区内断裂、裂隙发育,共同决定了斑岩-矽卡岩系统的产出。  相似文献   

A Model Atmosphere Analysis of the F6V Star π3 Ori     

A. Ajabshirizadeh  A. Muradov  Z. Samedov 《Astrophysics and Space Science》2004,293(3):289-294

Model atmosphere analysis, based on Kurucz models has been applied to study the F6V star π³ Ori (=BS1543=HD30652). The following values of the effective temperature, surface gravity and microturbulence velocity were obtained: = 6270±200 K, log g = 3.80.2, ξ_t =3.5±0.5 km/s. The abundances of 10 elements were determined. The resulting element abundances for the π³ Ori were found to be about three times lower with respect to the Sun. From evolutionary calculations we derived a mass, radius and luminosity for π³ Ori of M =1.3 M_⊙, R =2.38 R_⊙, L =7.9 L_⊙. Hence this star should be classified F6IV instead of F6 V. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

3. Solar System Formation and Early Evolution: the First 100 Million Years     

Thierry Montmerle  Jean-Charles Augereau  Marc Chaussidon  Mathieu Gounelle  Bernard Marty  Alessandro Morbidelli 《Earth, Moon, and Planets》2006,98(1-4):39-95

The solar system, as we know it today, is about 4.5 billion years old. It is widely believed that it was essentially completed 100 million years after the formation of the Sun, which itself took less than 1 million years, although the exact chronology remains highly uncertain. For instance: which, of the giant planets or the terrestrial planets, formed first, and how? How did they acquire their mass? What was the early evolution of the “primitive solar nebula” (solar nebula for short)? What is its relation with the circumstellar disks that are ubiquitous around young low-mass stars today? Is it possible to define a “time zero” (t ₀), the epoch of the formation of the solar system? Is the solar system exceptional or common? This astronomical chapter focuses on the early stages, which determine in large part the subsequent evolution of the proto-solar system. This evolution is logarithmic, being very fast initially, then gradually slowing down. The chapter is thus divided in three parts: (1) The first million years: the stellar era. The dominant phase is the formation of the Sun in a stellar cluster, via accretion of material from a circumstellar disk, itself fed by a progressively vanishing circumstellar envelope. (2) The first 10 million years: the disk era. The dominant phase is the evolution and progressive disappearance of circumstellar disks around evolved young stars; planets will start to form at this stage. Important constraints on the solar nebula and on planet formation are drawn from the most primitive objects in the solar system, i.e., meteorites. (3) The first 100 million years: the “telluric” era. This phase is dominated by terrestrial (rocky) planet formation and differentiation, and the appearance of oceans and atmospheres.  相似文献   

Cosmic Ray Acceleration Inside Molecular Clouds     

V. A. Dogiel  A. V. Gurevich  Ya. N. Istomin  K. P. Zybin 《Astrophysics and Space Science》2005,297(1-4):201-211

Acceleration of charged particles by neutral gas turbulence in giant molecular clouds is considered. The gamma-ray emission from these clouds is estimated. It is shown that molecular clouds can be the counterparts of some of unidentified sources.  相似文献   

Characteristics of rapid giant landslides in China   总被引：1，自引：0，他引：1  

Baoping?WenEmail author  Sijing?Wang  Enzhi?Wang  Jianmin?Zhang 《Landslides》2004,1(4):247-261

Factual data for 70 rapid, giant landslides since 1900 show that the occurrence of these landslides was largely predisposed by tectonics, geological structures, lithology and topography, and often triggered by rainfall and earthquakes. In terms of mobile behavior, the giant landslides can be classified into three types: slides, slide-flows and flows. It is found that each type of landslide was constrained to certain geologic and topographic regimes. There are good correlations between kinematic parameters of landslides and slope geometries, which confirm the important role played by topographical condition in the mobile behavior of landslides. Moreover, it is also found that each type of landslide presents distinct geotechnical characteristics in terms of nature of the slip zone and properties of sliding mass. Brief analyses of five typical cases illustrate that landslide mechanisms can be conceptually depicted by failure mechanisms of their slip zones prior to onset of movement and following energy conversion during movement. Problems and questions related to experience in China suggest that comprehensive and systematic investigation and study on rapid giant landslides are urgently needed.  相似文献   

LABORATORY OBSERVATIONS OF SEDIMENT ENTRAINMENT BY FREEZING SUPERCOOLED WATER     

SIMON J. COOK  PETER G. KNIGHT  DEBORAH A. KNIGHT  RICHARD I. WALLER 《Geografiska Annaler: Series A, Physical Geography》2012,94(3):351-362

Debris in basal ice produced by glaciohydraulic supercooling is typically characterized by high proportions of silt. A prominent hypothesis for this silt‐dominance is that frazil ice growing in supercooled water preferentially traps silt from sediment‐laden water percolating through it. It has therefore been suggested that silt‐dominance may be diagnostic of glaciohydraulic supercooling. The aim of our work is to test this hypothesis that freezing sediment‐laden supercooled water necessarily produces ice dominated by silt. We do this by simulating two freezing processes under laboratory conditions: (1) percolation of sediment‐laden water through frazil ice; (2) turbulent supercooling and subsequent freezing of sediment‐laden water. In experiments repeated using different particle sizes (sand, silt and clay in individual experiments) both processes entrained sand most effectively and silt least effectively. In experiments using a sediment mixture dominated by medium to coarse silt, both processes produced ice facies dominated by particle sizes between fine sand and coarse silt. These results suggest that silt‐dominance should therefore not be expected for supercooled freeze‐on, and is not a reliable diagnostic signature for supercooling. The silt‐dominated character of basal ice types associated with supercooling may result from other controls such as a silt‐dominated sediment supply or subglacial water flow rates, rather than the freezing process.  相似文献   

静力作用下夯土遗址根部掏蚀失稳机制实验研究   总被引：1，自引：1，他引：0       下载免费PDF全文

张博  谌文武  裴强强  赵建忠  石玉成  王旭东  郭青林 《地震工程学报》2021,43(2):430-437

根部掏蚀是土遗址坍塌的主要因素。关于土遗址掏蚀失稳机理已有众多研究成果,但主要基于数值模拟和理论分析,等比例进行根部掏蚀实验的研究较少。基于夯土遗址掏蚀调查研究,制作1∶1夯土墙体模型,通过墙体根部掏蚀实验和数值模拟对其失稳机制进行研究。实验结果表明:掏蚀深度小于20%时,墙体应力变化很小;掏蚀深度大于20%时,墙体出现偏应力,并且快速增大;掏蚀深度为45%时,墙体发生倾倒破坏。在实验过程中,墙体应力重分布主要发生在掏蚀阶段,掏蚀稳定后应力变化不明显;墙体倾倒破坏过程非常迅速,整体表现为刚性倾倒,从夯层根部层界面拉裂是主要破坏模式,其应力应变特征与数值模拟结果相吻合。研究成果可为夯土遗址根部保护和夯筑支顶加固提供参考依据。  相似文献   

Giant Mineral Deposits and Their Geodynamic Setting in the Lanping Basin, Yunnan, China   总被引：6，自引：0，他引：6  

XUE Chunji  LIU Shuwen  CHEN Yuchuan  ZENG Rong  ZHAO Shihua College of Earth Sciences  Resources  Chang''an University  Xi''an  Shaanxi  Chinese Academy of Geological Sciences  Beijing 《《地质学报》英文版》2004,78(2):368-374

There are giant mineral deposits, including the Jinding Zn-Pb and Baiyangping Ag-Co-Cu, and otherimportant mineral deposits (e.g., Baiyangchang Ag-Cu, Jinman Cu deposits, etc.) in the Lanping Mesozoic-Cenozoic Basin, Yunnan Province, China. The tabular ore-bodies and some veins hosted in terrestrial clastic rocks of the Mesozoic-Cenozoic age and no outcropping of igneous rocks in the giant deposits lead to the proposal of syngenetic origin, but the giant mineral deposits are not stratabound (e.g. MVT, sandstone- and Sedex-type). They formed in a continental red basin with intense crust movement. The mineralization is controlled by structures and lithology and occurs in different strata, and no sedimentary nature and no exhalative sediments are identified in the deposits. The deposits show some relations with organic matter (now asphalt and petroleum) and evaporates (gypsum). The middle-low-temperature (mainly 110℃ to 280℃) mineralization took place at a depth of about 0.9 km to 3.1 km during the early  相似文献   

钠基蒙脱土水合演化机制     

张云龙  项伟  黄伟  刘清秉  DAO Minh huan 《岩土力学》2019,40(11):4391-4400

为了查明钠基蒙脱土的水合演化过程,以天然钠基蒙脱土为研究对象,开展在相对湿度（ ）为0～0.98区间的水汽等温吸-脱附试验,通过吸附速率曲线、BET曲线界定钠基蒙脱土各水合阶段及相应的水合主控因素;通过测定晶层 值变化规律,从吸附水影响黏土矿物晶层厚度的角度探讨钠基蒙脱土的水合演化特征;基于傅里叶红外光谱,从水分子结构伸缩振动信息角度对钠基蒙脱土水合演化过程进行定性定量验证;通过热重/差热分析,以吸附水相变所需能量与吸附水重量变化的角度解释钠基蒙脱土的吸附水特征与其水合机制的关系。试验结果表明：在较低相对湿度下（0 0.15）,以钠基蒙脱土矿物外表面吸附为主,形成表面吸附水;0.15 0.40为钠基蒙脱土层间阳离子水合阶段;0.40 0.98,为晶层内外表面水合阶段,水分子逐步完整的包裹蒙脱土,形成多层吸附层。钠基蒙脱土的水合演化过程受控于层间钠离子与晶层基面,层间钠离子的水合能影响了钠基蒙脱土水合演化的起始顺序。  相似文献