O-rich SR and Mira variables in DENIS

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.     

阿尔泰南缘地球物理场特征与矿床分布规律

通过对新疆阿尔泰南缘地球物理场特征-深部构造-已知大型矿床分布规律的系统研究,认为该地区不同属性的地质块体受3组基底构造控制,即EW向、NE向和NW向3组基底构造系,并认为该地区已知大型-超大型矿床同样受这3组深部构造系的控制.最后对阿尔泰地区进行了大型、超大型多金属矿床成矿预测.     

Study on Yanshanian metallogenic granitoids magmatism in Baoshan deposit,southern Hunan ProvinceSCIEI北大核心CSCD

本文对湘南宝山花岗闪长斑岩进行了系统的锆石和磷灰石U-Pb定年、岩石地球化学以及锆石Hf同位素研究,并探讨了宝山花岗闪长斑岩的岩石成因和构造意义。锆石和磷灰石的LA-ICP-MS U-Pb定年显示,宝山花岗闪长斑岩的成岩年龄为160Ma。综合元素和同位素地球化学证据,宝山花岗闪长斑岩的成因可能为新生地壳与古老地壳的混合熔融,同时宝山花岗闪长斑岩中发现的890±20Ma的继承锆石,验证了新元古代新生地壳的参与。磷灰石的主微量元素研究显示花岗闪长斑岩具有较高的氧逸度和Cl含量,Sr/Th比值具有较大变化,而La/Sm比值变化不大等特征,表明形成花岗闪长斑岩岩浆的母岩受到俯冲板片脱水形成的流体交代作用影响。在上述过程中,富含Cl和H2O的流体从板片中释放出来,引发地幔楔熔融,并对矿床中成矿金属元素进行提取。由于古太平洋板块俯冲引发的伸展-减薄运动,在地幔上涌过程中,新元古代新生地壳发生部分熔融,这些高温岩浆底侵老地壳源区,诱发老地壳部分熔融,进而发生了强烈的壳-壳混合作用,产生花岗闪长质岩浆。     

Magmatic control on the contrasting Sn feritility of different granite plutons in the giant Gejiu orefield.SCIEI北大核心CSCD

云南个旧锡矿是全球最大的锡多金属矿床之一,但矿区内同时代花岗岩成锡矿潜力差异显著,其控制因素仍不清楚。本文选取贫矿的龙岔河似斑状花岗岩和成锡矿的老厂-卡房(后文简称老-卡)花岗岩为研究对象,通过全岩地球化学成分和黑云母成分分析,系统研究个旧矿区不同花岗岩成锡矿潜力差异的控制因素。测试结果表明,龙岔河花岗岩和老-卡花岗岩具有相似的、以表壳物质为主的岩浆源区以及较高的初始熔融温度,表明岩浆源区和熔融条件不是控制二者成矿潜力差异的主要原因。黑云母成分显示老-卡花岗岩和龙岔河花岗岩均具有较低的氧逸度,岩浆演化过程中锡为不相容元素,有利于锡在残余熔体中富集,表明氧逸度条件也不是导致成矿潜力差异的关键因素。龙岔河花岗岩发育角闪石、榍石、黑云母,而老-卡花岗岩发育岩浆白云母,指示后者分异程度更高。此外,与龙岔河花岗岩相比,老-卡花岗岩具有富硅,贫钛、铁、镁、钙和稀土元素特征,稀土元素呈现“海鸥式”配分模式,并且具有较低的Nb/Ta、Zr/Hf、K/Rb和较高的Rb/Sr比值,同样指示老-卡花岗岩具有更高的结晶分异程度。并且相比于龙岔河花岗岩为准铝质的特征,老-卡花岗岩的过铝质特征有利于锡分配进入岩浆出溶的流体相中富集成矿。因此,岩浆性质和演化程度是导致个旧地区不同花岗岩成矿潜力差异的主要原因,龙岔河花岗岩形成锡矿化的潜力较小。     

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

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。     

A Model Atmosphere Analysis of the F6V Star π3 Ori

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.     

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

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.     

Cosmic Ray Acceleration Inside Molecular Clouds

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.     

欧亚黄土沉积环境对比研究

本文对采自中国、法国、比利时等国43块黄土样品进行实验室处理后,分析对比了它们在碳酸盐含量、粒度组成、重矿物组成及粘土矿物成分方面的共同特性及差异性。结果表明,中国黄土碳酸盐含量稳定,西欧不同类型的黄土碳酸盐含量差别很大。在粒度组成上,欧亚黄土并没有本质的差别,但西欧不同层位的黄土粒度组成呈有规律变化。对西欧重矿物的分析可以追溯黄土的物质来源,粘土矿物含量在欧亚不同黄土中也有差别。比较结果说明,欧洲的黄土堆积受第四纪冰期、间冰期的气候波动影响较大,中国黄土在堆积期间始终处在干旱、半干旱的气候条件下。