On the physical connections between galaxies of different types

Galaxies can be classified in two broad sequences which are likely to reflect their formation mechanism. The 'main sequence', consisting of spirals, irregulars and all dwarf galaxies, is probably produced by gas settling within dark matter haloes. We show that the sizes and surface densities along this sequence are primarily determined by the distributions of the angular momentum and formation time of dark haloes. They are well reproduced by current cosmogonies provided that galaxies form late, at z  ≲ 2. In this scenario, dwarf ellipticals were small 'discs' at z  ∼ 1 and become 'ellipticals' after they fall into cluster environments. The strong clustering of dwarf ellipticals is then a natural by-product of the merging and transformation process. The number of dwarf galaxies predicted in a cluster such as Virgo is in good agreement with the observed number. On the other hand, the 'giant branch', consisting of giant ellipticals and bulges, is probably produced by the merging of disc galaxies. Based on the observed phase-space densities of galaxies, we show that the main bodies of all giant ellipticals can be produced by dissipationless mergers of high-redshift discs. However, high-redshift discs, although denser than present-day ones, are still not compact enough to produce the high central phase-space density of some low-luminosity ellipticals. Dissipation must have occurred in the central parts of these galaxies during the merger which formed them.     

Star forming activities in W75N and DR21 – Are the two regions in collision?

We have observed the massive star formation region W75N in ¹²CO J = 3 ? 2 with KOSMA. The profile of ¹²CO J = 3 ? 2 indicated that besides the 9 km s^?1 component, there is another component of ?3 km s^?1, which is associated with another star formation region, DR21N, located to the north of DR21. We derived the physical and dynamical parameters of the core and high velocity gas associated with the two components separately. Star forming activities were investigated, including outflows and infall analysis. The two regions overlap in space and are not connected in velocity. We found that the cloud–cloud collision scenario may not apply for the DR21/W75N case.     

Precise Synchrotron Radiation Spectrum of Fast-cooling Electrons and the Prompt GRB Emission

It is generally believed that the synchrotron radiation of electrons from the internal shock is the main radiation mechanism of the prompt GRB (gamma-ray burst) emission. However, what this model predicts can not explain observations well. In this paper, we confirm that electrons are quickly cooled due to radiation losses and also point out that the synchrotron radiation spectrum presented in previous papers is a relatively rough estimation. We get the precise synchrotron radiation spectrum of fast-cooling electrons by carrying out a numerical calculation, and thereby reasonably explain the observed distribution of low-energy spectral index (α) of long GRBs based on a unified model. In addition, we fit the correlation between α and the peak energy of the νFν spectrum (E_p).     

Feedback of Active Galactic Nuclei in Seyfert 2 Galaxies

It is well accepted that feedback from active galactic nuclei (AGNs) plays an important role in the coevolution of the supermassive black hole (SMBH) and its host galaxy,but the concrete mechanism of feedback remains unclear.A considerable body of evidence suggests that AGN feedback suppresses star formation in the host galaxy.We assemble a sample of Seyfert 2 galaxies with recent observational data of compact nuclear starbursts and estimate the gas surface density as a function of column density to illuminate the relation between feedback and AGN properties.Although there are some uncertainties,our data still imply the deviation from the star formation law (Kennicutt-Schmidt law).Further,they indicate that:(1) Feedback correlates with the Eddington ratio,rather than with the mass of SMBH,as a result of decreasing star formation efficiency.(2) The SMBH and the torus are probably undergoing coevolution.Conclusions presented here can be refined through future high resolution CO or HCN observations.     

二安替比林基—（2—溴）苯基甲烷与铈的显色反应及应用

合成了二安替比林基＿（２＿溴）苯基甲烷（ＤＡｏＢＭ）。在Ｍｎ（Ⅱ）和吐温＿８０存在下,Ｃｅ（Ⅳ）与ＤＡｏＢＭ反应生成有色化合物,λｍａｘ为４８０ｎｍ,摩尔吸光系数为３１×１０５Ｌ·ｍｏｌ－１·ｃｍ－１。Ｃｅ（Ⅳ）的质量浓度为０００４～０２ｍｇ／Ｌ时符合比尔定律。方法已用于稀土矿石中微量Ｃｅ（Ⅳ）的测定,结果与ＩＣＰ＿ＡＥＳ法相符     

Geochemical anomaly structure of South Mining District of Fenghuangshan Copper Mine

To study the geochemical anomaly structure of multi-element associations in the South Mining District of the Fenghuangshan Copper Mine,samples were collected and analyzed for their trace element contents.Multi-element anomaly associations were divided according to the correlations between Cu and each of the other elements,and the distribution characteristics of multi-element anomaly associations were also described.Among them,the anomaly distribution of metallogenic element Cu indicates the environment of mineralization.This study provided the basis for research on the metallogenic prediction and geochemistry of the Fenghuangshan Copper Mine.     

埋藏第四系的沉积相研究——地球物理测井解释在第四纪沉积研究中的应用

关于第四纪埋藏沉积物成因类型的研究,常规的方法是利用钻井取芯资料进行综合分析和对比,所得结论往往是定性的。由于钻井取芯的费用十分昂贵,且第四纪松散沉积物的收获率一般比较低,所以这种方法的广泛应用受到了很大的限制。本文介绍了一种利用测井资料进行沉积相分析的思路和方法。由于地球物理测井具有快速、经济等特点,因此该方法在第四纪沉积的研究中具有较好的应用前景。另外,随着计算机的广泛使用,人工智能技术的迅速发展为测井相分析的定量化和自动化提供了实现的途径。     

Masses for free-floating planets and dwarf planets

The mass and distance functions of free-floating planets(FFPs) would give major insights into the formation and evolution of planetary systems, including any systematic differences between those in the disk and bulge. We show that the only way to measure the mass and distance of individual FFPs over a broad range of distances is to observe them simultaneously from two observatories separated by D ～ O(0.01 au)(to measure their microlens parallax π_E) and to focus on the finite-source point-lens(FSPL) events(which yield the Einstein radius θ_E). By combining the existing KMTNet 3-telescope observatory with a 0.3 m 4 deg~2 telescope at L2, of order 130 such measurements could be made over four years, down to about M ～ 6 M_⊕for bulge FFPs and M ～ 0.7 M_⊕for disk FFPs. The same experiment would return masses and distances for many bound planetary systems. A more ambitious experiment, with two 0.5 m satellites(one at L2 and the other nearer Earth) and similar camera layout but in the infrared, could measure masses and distances of sub-Moon mass objects, and thereby probe(and distinguish between) genuine sub-Moon FFPs and sub-Moon "dwarf planets" in exo-Kuiper Belts and exo-Oort Clouds.     

利用FME的CAD在数据不同基准坐标系之间的变换

对坐标系统转换和变换进行总结,并分析了平面坐标系坐标变换问题和不同基准数据的坐标变换问题。针对CAD地形数据的基准变换问题,利用FME Desktop软件实现CAD数据不同基准下不同坐标形式的变换。     

苏南地区城乡聚落空间演化过程及其格局特征

当前,城乡聚落空间正由自然和经济社会条件存在差异的等级体系转变为密切联系的网络化结构,城乡融合已经成为中国城乡聚落空间演化发展的重要方向。以苏南地区为例,对20世纪90年代以来的城乡聚落空间演化过程及其格局特征进行分析,发现2000年以后城镇聚落扩张强度远高于乡村聚落,城乡聚落空间结构可进一步归纳为集中、双心、多核和密集4种基本格局。该研究对乡村振兴背景下的城乡聚落空间优化布局具有一定指导作用。