Tidal evolution of discy dwarf galaxies in the Milky Way potential: the formation of dwarf spheroidals     

Jaros&#;aw Klimentowski  Ewa L. &#;okas  Stelios Kazantzidis  Lucio Mayer  Gary A. Mamon 《Monthly notices of the Royal Astronomical Society》2009,397(4):2015-2029

We conduct high-resolution collisionless N -body simulations to investigate the tidal evolution of dwarf galaxies on an eccentric orbit in the Milky Way (MW) potential. The dwarfs originally consist of a low surface brightness stellar disc embedded in a cosmologically motivated dark matter halo. During 10 Gyr of dynamical evolution and after five pericentre passages, the dwarfs suffer substantial mass loss and their stellar component undergoes a major morphological transformation from a disc to a bar and finally to a spheroid. The bar is preserved for most of the time as the angular momentum is transferred outside the galaxy. A dwarf spheroidal (dSph) galaxy is formed via gradual shortening of the bar. This work thus provides a comprehensive quantitative explanation of a potentially crucial morphological transformation mechanism for dwarf galaxies that operates in groups as well as in clusters. We compare three cases with different initial inclinations of the disc and find that the evolution is fastest when the disc is coplanar with the orbit. Despite the strong tidal perturbations and mass loss, the dwarfs remain dark matter dominated. For most of the time, the one-dimensional stellar velocity dispersion, σ, follows the maximum circular velocity, V _max, and they are both good tracers of the bound mass. Specifically, we find that   M _bound∝ V ^3.5_max  and     in agreement with earlier studies based on pure dark matter simulations. The latter relation is based on directly measuring the stellar kinematics of the simulated dwarf, and may thus be reliably used to map the observed stellar velocity dispersions of dSphs to halo circular velocities when addressing the missing satellites problem.  相似文献   

一种起伏地表条件下的照明补偿方法          下载免费PDF全文

叶月明  吴如山  范国章  丁仁伟 《地球物理学报》2021,64(1):224-232

起伏的地表条件限制了采集孔径范围并造成深层地震照明不足,为改善该类地区的成像质量,本文提出了一种起伏地表条件下的照明补偿方法.首先,基于小波束波场延拓算子和逐步累加的外推方法在波场延拓过程中解决起伏地表面的影响,并引入空间滤波函数压制虚拟层内的偏移噪音;其次,利用局部指数标架对上、下行波场分解,得到局部角度域成像和照明补偿因子.再次,利用计算出的成像值和照明补偿因子,在局部倾角域完成照明补偿.SEG起伏地表模型测试证明了本方法的有效性,深层构造照明度明显加强,不同角度成像振幅更加均衡,该技术为提高起伏地表地区的成像品质提供了新的手段.  相似文献   

Investigation of local time dependence of Mercury's sodium exosphere based on a numerical simulation     

Hiroaki Misawa  Aya Sonobe  Akira Morioka 《Planetary and Space Science》2008,56(13):1681-1687

Mercury has a surface-bounded exosphere (SBE) similar to that of the Moon. One of the atmospheric species, sodium, was found by ground-based observations to be the most prominent component. Mercury's sodium SBE is known to be non-uniform with respect to local time (LT) in low-latitude regions: the sodium column density in the dawn-side region is larger than that in the dusk-side region, and the sodium abundance is the largest in the morning-noon region. To reveal the production processes for the exosphere near Mercury's surface, the LT dependence of the exosphere was investigated through a numerical simulation. Three data sets of sodium column densities observed for the dawn-side hemisphere, observed by Sprague et al. [1997. Distribution and abundance of sodium in Mercury's atmosphere, 1985-1988. Icarus 12, 506-527], were compared with results simulated by a 3D Monte Carlo method, and the source rates and density of sodium of the planetary surface were estimated. In the simulation, the photon-stimulated desorption (PSD) and thermal desorption (TD) processes were assumed as the release mechanisms. The sodium source rates for the three data sets, at respective heliocentric distances of about 0.33, 0.42, and 0.44 AU, were estimated as 1-4×10⁸ Na/cm²/s with weak LT dependence. In contrast, the expected sodium surface density showed clear dependence on LT and the heliocentric distance. The sodium surface density decreases from early morning to noon by a few orders, and, particularly for large heliocentric distances, the surface is in a condition of sodium excess and depletion with respect to the surface sodium density assumed by Killen et al. [2004. Source rates and ion recycling rates for Na and K in Mercury's atmosphere. Icarus 171, 1-19] in the early morning and morning-noon regions, respectively. This study implies that the decrease in sodium surface density from the early morning to noon regions might produce the characteristic LT dependence in the low-latitude dawn-side region.  相似文献   

The local Hubble flow: is it a manifestation of dark energy?     

Yehuda Hoffman  Luis A. Martinez-Vaquero  Gustavo Yepes  Stefan Gottlöber 《Monthly notices of the Royal Astronomical Society》2008,386(1):390-396

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Research on Initial Modeling Method for TTI Anisotropic Parameters Based on Local Tomography     

Kai Guo 《地球科学进展》2019,34(10):1060-1068

The initial modeling method based on TTI anisotropy can provide an initial model for the fine modeling of tomographic inversion, and the quality of the initial model directly affects the efficiency and accuracy of tomographic inversion. It is necessary to study the accurate initial modeling method of TTI anisotropy. Based on the conventional flow of the initial modeling method of TTI anisotropic, in this paper the anisotropic parameter extraction formula was perfected, a local tomography method to optimize the flow of the initial modeling method of TTI anisotropy was introduced, and the accuracy of the initial model was further improved, which is more consistent with the actual geological conditions and conducive to the fine modeling of the later tomographic inversion. The processing results of model and filed data show that the initial modeling method of TTI anisotropy based on local tomography is effective and practical.  相似文献   

Precise Determination of Astronomical Azimuth by the Hour Angle Method of Multiple Meridian Stars     

《Chinese Astronomy and Astrophysics》2020,44(4):536-548

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基于LSH方法的珊瑚礁鱼类竞争压力查询和资源分配方法     

赵丹枫  黄洲  许强  黄冬梅 《热带海洋学报》2020,39(2):118-126

基于海洋大数据查询技术的珊瑚礁鱼类保护策略是海洋科学研究的重要课题, 其中鱼群竞争状况对鱼类保护具有重要意义。研究鱼群竞争状况就必须模型化鱼群与珊瑚礁的依赖关系。作为一个简单有效的大数据模型, 图模型是表达这个关系的实用模型。文章提出表达珊瑚礁鱼类种群和珊瑚礁资源依赖关系的竞争图建模方法, 并提出基于局部敏感哈希(Local Sensitive Hashing, LSH)的鱼类种群竞争压力竞争图查询方法, 得到鱼类种群的实时竞争压力状况; 然后根据LSH查询结果, 分析出需要优先保护的鱼类种群; 最后对这些需要优先保护的鱼类种群设计了基于构建人工礁的资源分配方法, 使得区域内珊瑚礁鱼类总体竞争状况改善。  相似文献   

QSOs behind the Milky Way satellite galaxies -- II     

C. G. Tinney 《Monthly notices of the Royal Astronomical Society》1999,303(3):565-574

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台风移动规律的研究 Ⅰ.非绝热加热与水平温度分布的影响   总被引：1，自引：1，他引：0  

贺海晏 《热带气象学报》1995,(1):1-9

根据大气运动原始方程组导出一个支配台风中心移动的基本方程。方程中包括了非绝热加热、温度场分布、地形与摩擦等各种可能影响台风移动的强迫因子。对非绝热加热与水平温度分布的作用所作分析表明,非轴对称的非绝热引导作用可使台风加速、减速或转向运动;温度场上的冷区对台风有吸引作用。   相似文献   

UBV and vbyβ stellar photometry in the eastern part of M31     

R.G. Kurtev 《Astronomische Nachrichten》2003,324(3):265-270

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