Orbital motion of a massive object in a dense stellar system

In this paper we show the positional oscillation of a massive object in a dense stellar system by numerical N -body simulations. We found that the central massive object, which at first is placed at rest at the centre of the surrounding spherical stellar system, promptly departs from the centre and rotates in accordance with the rotation of the stellar system, if the stellar system has an appreciable rotation. This oscillatory motion continues for a long time because of the absence of dynamical friction. Such a long-lasting oscillation may explain the asymmetric structure observed in the centres of M31 and NGC 4486B, may cause the secular flow of gaseous elements distributed in the central regions of galaxies on to the massive object, and may ignite activity in the centres of galaxies.     

澳大利亚拉克兰造山带成矿地质条件与主要矿化类型

澳大利亚拉克兰造山带（又称拉克兰褶皱带,简称LFB）由强烈变形的寒武纪—泥盆纪深海沉积岩、燧石和基性火山岩,以及更年轻的盖层所构成,其造山过程表现为澳大利亚板块向东南方向不断增生的过程。该造山带的长期演化,形成了以维多利亚金矿省为典型代表的造山型金矿床及其它类型的多金属矿床,本质上这些矿床的形成与特殊的成矿地质条件密切相关。对该区相关文献进行分析和总结,提炼出拉克兰造山带金及多金属矿床的主要地质特征,划分出5种主要矿化类型：造山型金矿、花岗岩中细脉浸染型钨—锡矿、斑岩型铜—金矿、火山喷流铜—锌—金硫化物矿床、产于断陷盆地沉积岩中的铜—铅—锌—金矿。5种矿化类型各具特色,空间上有规律性地分布。     

The evolution of bodies orbiting in the trans-Neptunian region on to intermediate-type orbits

We investigate the dynamical evolution of 210 hypothetical massless bodies initially situated between 10 and 30 au from the Sun in order to determine the general characteristics of the evolved system. This is of particular relevance to the understanding of the origin of Edgeworth–Kuiper belt objects on scattered intermediate orbits, such as 1996 TL ₆₆, which have high eccentricity and semimajor axis but nevertheless have perihelion in the region between 30 and 50 au from the Sun.     

东北典型丘陵漫岗区沟谷侵蚀动态及空间分析

以黑龙江省克山县为例,分析1954年和2000年侵蚀沟密度变化,探讨研究区土壤侵蚀的时空动态变化,并以侵蚀沟密度变化值为依据进行不同分区侵蚀因素的耦合分析。结果表明:过去46年间,克山县东南部侵蚀沟密度趋于减少,西北部侵蚀沟密度增大。1954～2000年侵蚀沟密度变化值在侵蚀减弱区与高程和坡度呈负相关,在侵蚀增强区呈正相关。随着坡长增加,侵蚀沟密度变化量呈增加趋势。侵蚀沟变化与坡长相关性最大,R²达0.9743,其次为高程,R²为0.6893,与坡度的相关性最小,R²为0.3437。结果表明,高程和坡度不是东北丘陵漫岗地区土壤流失的主要影响因子,坡长是该区侵蚀的一个重要影响因子。土地利用结构变化与土壤侵蚀强度变化密切相关,耕地面积大幅度增加与草地面积明显减少加速侵蚀沟发育。     

On Relativistic Equations of Motion of an Earth Satellite

For numerical integration of the geocentric equations of motion of Earth satellites in the general relativity framework one may choose now between rather simple equations involving in their relativistic dynamical part only the Earth-induced terms and very complicated equations taking into account the relativistic third-body action. However, it is possible quite easily to take into account the relativistic indirect third-body perturbations and to neglect much lesser direct third-body perturbations. Such approach is based on the use of the Newtonian third-body perturbations in geocentric variables with expressing them in the relativistic manner in terms of the barycentric arguments. Together with it, to extend the known results for the spheroid model of the Earth, the Earth-induced terms are treated in great detail by including the non-spin part of the Earth vector-potential and the Earth triaxial non-sphericity.This revised version was published online in October 2005 with corrections to the Cover Date.     

鄂东南地区印支期以来构造变形特征及油气意义

利用区域地震大剖面及MT资料,结合地面地质调查成果,对鄂东南地区的深部地质结构及典型构造样式进行了分析,认为该区发育以基底岩系顶面和志留系顶面为主滑脱面的大型逆冲推覆构造,并识别出双重逆冲构造、叠瓦状构造、台阶式结构、对冲构造及反冲断层等典型构造样式;同时对上下地质结构的变异进行了探讨,提出志留系滑脱层之下的“原地体”具有变形相对较弱、褶皱宽缓开阔的特点,在后期拉张改造中受到上盘“异地体”的保护,应是有利的油气勘探领域,双重逆冲构造内部发育的断层相关褶皱(如随阳构造)是重点勘探目标。     

Modelling the bar in the centre of the starburst galaxy M82

We present VLA A-array 21-cm atomic hydrogen (H  i ) absorption observed against the central region of the starburst galaxy M82 with an angular resolution of ∼1.3 arcsec (≃20 pc). These observations, together with MERLIN H  i absorption measurements, are compared with the molecular (CO) and ionized ([Ne  ii ]) gas distributions and are used to constrain the dynamics and structure of the ionized, neutral and molecular gas in this starburst.
A position–velocity diagram of the H  i distribution reveals an unusual 'hole' feature which, when previously observed in CO, has been interpreted as an expanding superbubble contained within a ring of gas in solid body rotation. However, we interpret this feature as a signature of a nearly edge-on barred galaxy. In addition, we note that the CO, H  i and [Ne  ii ] position–velocity diagrams reveal two main velocity gradients, and we interpret these as gas moving on x₁- and x₂-orbits within a bar potential. We find the best fit to the data to be produced using a bar potential with a flat rotation curve velocity v _b=140 km s⁻¹ and a total length of 1 kpc, a non-axisymmetry parameter q =0.9, an angular velocity of the bar Ω_b=217 km s⁻¹ arcsec⁻¹, a core radius R _c=25 pc, an inclination angle i =80° and a projected angle between the bar and the major axis of the galaxy φ '=4°. We also discuss the orientation of the disc and bar in M82.     

耿达短水准异常与汶川8.0级地震

结合龙门山断裂带其他跨断层资料,对耿达短水准在汶川8.0级地震前后的观测资料进行了重新分析,发现耿达短水准在汶川地震前后的异常为当地居民修建生活小区所致,不应视为地震前兆异常。     

Crustal structure across the Grand Banks–Newfoundland Basin Continental Margin – II. Results from a seismic reflection profile

New multichannel seismic reflection data were collected over a 565 km transect covering the non-volcanic rifted margin of the central eastern Grand Banks and the Newfoundland Basin in the northwestern Atlantic. Three major crustal zones are interpreted from west to east over the seaward 350 km of the profile: (1) continental crust; (2) transitional basement and (3) oceanic crust. Continental crust thins over a wide zone (∼160 km) by forming a large rift basin (Carson Basin) and seaward fault block, together with a series of smaller fault blocks eastwards beneath the Salar and Newfoundland basins. Analysis of selected previous reflection profiles (Lithoprobe 85-4, 85-2 and Conrad NB-1) indicates that prominent landward-dipping reflections observed under the continental slope are a regional phenomenon. They define the landward edge of a deep serpentinized mantle layer, which underlies both extended continental crust and transitional basement. The 80-km-wide transitional basement is defined landwards by a basement high that may consist of serpentinized peridotite and seawards by a pair of basement highs of unknown crustal origin. Flat and unreflective transitional basement most likely is exhumed, serpentinized mantle, although our results do not exclude the possibility of anomalously thinned oceanic crust. A Moho reflection below interpreted oceanic crust is first observed landwards of magnetic anomaly M4, 230 km from the shelf break. Extrapolation of ages from chron M0 to the edge of interpreted oceanic crust suggests that the onset of seafloor spreading was ∼138 Ma (Valanginian) in the south (southern Newfoundland Basin) to ∼125 Ma (Barremian–Aptian boundary) in the north (Flemish Cap), comparable to those proposed for the conjugate margins.     

亚热带4种行道树树干表面CO_2释放速率昼夜动态

采用LI-8100土壤碳通量自动测量系统,与自制的树干呼吸观测气室相连,原位观测亚热带春、秋2个季节4种行道树树干呼吸速率及相关环境因子的昼夜动态.结果表明:在秋季土壤水分较低水平下(VWC平均为11.6%),羊蹄甲、香樟树干呼吸速率昼夜动态呈单峰曲线,和温度变化呈极显著指数函数关系,峰值分别出现在17:00和13:00;芒果和高山榕树干呼吸速率昼夜动态单峰不明显,白天与树干温度变化呈极显著指数函数关系,但芒果白天与夜间的树干呼吸速率差异不显著,而高山榕树干呼吸速率夜间显著高于白天,二者出现"白昼抑制"现象.在春季土壤水分较高水平下(VWC平均为22.1%),羊蹄甲、芒果和高山榕树干呼吸速率昼夜动态呈单峰型曲线,峰值分别出现在11:00、15:00和14:00;而香樟树干呼吸速率单峰不明显,4种树种的树干呼吸速率昼夜动态均与温度变化呈极显著指数函数关系.2个季节中,树干温度与树干呼吸的指数函数关系最好,秋季羊蹄甲、芒果和香樟树干呼吸速率对树干昼夜温度变化的Q10值分别为2.04、2.37和2.18,春季羊蹄甲、芒果、香樟和高山榕树干呼吸速率对树干昼夜温度变化的Q10值分别为2.27、2.58、1.90和1.8...