The faint end of the galaxy luminosity function     

Neil Trentham  R. Brent Tully 《Monthly notices of the Royal Astronomical Society》2002,335(3):712-732

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变质岩的变质序列分析──以辽河群为例     

郭洪方 《国土资源》1994,(Z1)

通过对辽河群岩石中主要变质矿物的观察和研究，以岩石的变形历史作为变质结晶作用的相对时标，确定了矿物生长的时序特征及其演化过程。发现变质与变形既是有密切联系的又是各自独立的地质作用，辽河期的变形作用存在明显的３个变形幕，而辽河期的变质作用是个连续的完整的过程，无明显的热波动。变质作用高峰和变形作用高峰存在时间差。  相似文献   

对二郎坪群火神庙组物质组成的质疑与再认识     

姜常义  苏生瑞  张振飞  杨志华  赵太平 《地球科学与环境学报》1995,(2)

经研究证明，前人建立的二郎坪群火神庙组确有少量的亚碱性双峰式火山岩。这些火山岩零星地分布在几个地区，走向不连续，出露宽度一般为数百米。构成该组主体的是一条规模宏伟的侵入岩带，其岩石组合为辉长岩－闪长岩－石英闪长岩－斜长花岗岩－花岗岩，总体上表现为正序岩浆演化序列。这些侵入岩普遍经历了三个阶段的变形变质作用，即第一阶段为韧性变形；第二阶段为静态重结晶；第三阶段为带状褶劈理，表现了复杂而漫长的构造演化史。  相似文献   

Giant HVC’s and the Rotation Curves of the Milky Way and M31     

E. Casuso  J. E. Beckman 《Astrophysics and Space Science》2006,306(3):139-145

We have modelled, for the cases of Milky Way and M31, the effects on the galactic discs, of the arrival at high velocity (≥150 km s⁻¹) of giant HI clouds, with masses of up to 10⁸M⊙. Predictions are compared with the detailed structure of the observed rotation curves for these two galaxies. The model explains the rises and falls observed at large distances from the centre of each galaxy, distributed with a degree of regularity in radius, in terms of a specific type of perturbations driven by the infall of the high velocity clouds (HVC's) arriving from the intracluster medium of the Local Group. The underlying rotation curve is explained conventionally via the distribution of the baryonic and dark matter components of the galaxy in question. This scenario, though tested here on the two major Local Group objects, is in principle applicable to galaxies undergoing minor mergers with subgalactic mass gas clouds.  相似文献   

A photometrically and kinematically distinct core in the Sextans dwarf spheroidal galaxy     

Jan T. Kleyna  Mark I. Wilkinson  N. Wyn Evans  Gerard Gilmore 《Monthly notices of the Royal Astronomical Society》2004,354(4):L66-L72

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论辽南上前寒武系的划分与对比   总被引：1，自引：0，他引：1  

段吉业  安素兰 《国土资源》1994,(Z1)

辽南上元古界的区域对比的关键是如何与蓟县层型、峡东层型的衔接或对比。作者认为辽南群是介于北方的青白口群与南方的震旦系之间的层位，仅金县群才相当于震旦系，震旦系与寒武系的界线则应置于兴民村组与葛屯组之间。  相似文献   

青田芝溪头鹤溪群浅变质岩系中发现动物化石     

朱德寿  胡耀华  石关根 《浙江国土资源》1994,(2)

作者于1993年4月在浙江青田芝溪头鹤溪群剖面上采集了白云质大理岩标本样品，送南京地质古生物研究所进行标本浸泡处理。首次获得鱼骨、管状化石及土菱子介等海相化石，经鉴定认为其时代可能属石岩—二叠纪。本文根据以往的同位素资料、沉积环境分析和区域对比，认为这套变质岩系的原岩为二叠纪含煤沉积岩，可与福建的童子岩组中上部层位对比。  相似文献   

甘肃陇山地区葫芦河群变质玄武岩及大地构造环境恢复   总被引：1，自引：0，他引：1  

樊双虎  张维吉  金符实  孟宪恂 《地球科学与环境学报》1993,(4)

葫芦河群变质玄武岩以其高不相容元素、稀土元素和低MgO、Cr和Ni含量有别于现代洋中脊玄武岩和岛弧玄武岩,在FeO-MgO-Al_2O_3和Ti/100-Zr-Y×3判别图上,均落在大陆玄武岩区。在剖面上,与变质玄武岩整合接触的巨厚的变砂岩和大量出现的火山角砾岩和集块岩是浅海环境的标志;密集的辉绿岩墙群是拉张性大地构造环境的特征。因此,本文认为葫芦河群变质玄武岩原岩形成于陆内裂陷海盆环境。  相似文献   

论本溪群     

范国清 《国土资源》1993,(2)

本溪群的原始定义属岩石地层单位,70年来的研究表明;其界线层型及岩百地层单位性质没有改变过;本溪群可以延展到东北南部及华北,并具有二分、三分的概分性。华北本溪群曾被划分为湖田组(铁铝岩组)和畔沟组,业已证实二分的可行性;张守信(1988,1992)欲以太原组(新涵义)替代本溪群(剔除下部铁铝岩组合)是不可行的。  相似文献   

Dark matter in dwarf spheroidals – II. Observations and modelling of Draco     

J.Kleyna  M. I.Wilkinson  N. W.Evans  G.Gilmore  C.Frayn 《Monthly notices of the Royal Astronomical Society》2002,330(4):792-806

We present stellar radial velocity data for the Draco dwarf spheroidal (dSph) galaxy obtained using the AF2/WYFFOS instrument combination on the William Herschel Telescope. Our data set consists of 186 member stars, 159 of which have good quality velocities, extending to a magnitude   V ≈19.5  with a mean velocity precision of ≈2 km s⁻¹. As this survey is based on a high-precision photometric target list, it contains many more Draco members at large radii. For the first time, this allows a robust determination of the radial behaviour of the velocity dispersion in a dSph.
We find statistically strong evidence of a rising velocity dispersion consistent with a dark matter halo that has a gently rising rotation curve. There is a <2 σ signature of rotation about the long axis, inconsistent with tidal disruption as the source of the rising dispersion. By comparing our data set with earlier velocities, we find that Draco probably has a binary distribution and fraction comparable to those in the solar neighbourhood.
We apply a novel maximum likelihood algorithm and fit the velocity data to a two parameter spherical model with an adjustable dark matter content and velocity anisotropy. Draco is best fit by a weakly tangentially anisotropic distribution of stellar orbits in a dark matter halo with a very slowly rising rotation law  ( v _circ∝ r ^0.17)  . We are able to rule out both a mass-follows-light distribution and an extended halo with a harmonic core at the 2.5 to 3 σ significance level, depending on the details of our assumptions about Draco's stellar binary population. Our modelling lends support to the idea that the dark matter in dwarf spheroidals is distributed in the form of massive, nearly isothermal haloes.  相似文献