Stellar and HI Mass Functions Predicted by a Simple Preheating Galaxy Formation Model     

Zhi-Jian Luo Cheng-Gang Shu 《中国天文和天体物理学报》2007,7(4):590-594

According to the new preheating mechanism of galaxy formation suggested by Mo et al., we construct a simple model of formation of disk galaxies within the current paradigm of galaxy formation. It incorporates preheating, gas cooling, bulge formation and star for-mation. The predicted stellar and HI mass functions of galaxies are discussed and compared with the observations. It is found that our model can roughly match both the observed galaxy luminosity function and the observed HI-mass function.  相似文献   

A Survey of Newtonian Core-Shell Systems with Pseudo High Order Symplectic Integrator and Fast Lyapunov Indicator     

Jun-Fang Zhu Xin Wu Da-Zhu Ma 《中国天文和天体物理学报》2007,7(4):601-610

Newtonian core-shell systems, as limiting cases of relativistic core-shell models under the two conditions of weak field and slow motion, could account for massive circumstellar dust shells and rings around certain types of star remnants. Because this kind of systems have Hamiltonians that can be split into a main part and a small perturbing part, a good choice of the numerical tool is the pseudo 8th order symplectic integrator of Laskar ＆ Robutel, and, to match the symplectic calculations, a good choice of chaos indicator is the fast Lyapunov indicator （FLI） with two nearby trajectories proposed by Wu, Huang ＆ Zhang. Numerical results show that the FLI is very powerful when describing not only the transition from regular motion to chaos but also the global structure of the phase space of the system.  相似文献   

Disk Thicknesses and Some Parameters of 108 Non-Edge-On Spiral Galaxies     

Tao Hu Qiu-He Peng Hong-Shi Zong 《中国天文和天体物理学报》2007,7(4):579-589

We present disk thicknesses, some other parameters and their statistics of 108 non-edge-on spiral galaxies. The method for determining the disk thickness is based on solving Poisson's equation for a disturbance of matter density in three-dimensional spiral galaxies. From the spiral arms found we could obtain the pitch angles, the inclination of the galactic disk, and the position of the innermost point (the forbidden region with radius r 0 to the galactic center) of the spiral arm, and finally the thickness.  相似文献   

1:5万区域化探样品分析测试的质量监控     

陈绳权 《华北国土资源》2009,(1)

依据《地质矿产实验室测试质量管理规范》,并结合山西省的地质情况建立了一套1:5万区域化探样品分析测试的质量监控体系。分四个部分详细论述了的1:5万区域化探样品分析测试的质量监控体系。过去1:5万质量监控体系完全是靠人工进行,效率低下;本质量监控体系与过去相比,不但节省了大量的人力、物力,而且更加准确、迅速,更能适应1:5万质量监控大量数据处理的需要。  相似文献   

多季相混合像元部分分解特征的不透水面分类     

陈姣  黄远程  李朋飞 《测绘科学》2021,46(4):90-99

针对利用光谱混合分解提取不透水面特征通常受到端元类型和数量的限制,同时植被变化会影响估计精度的问题,该文提出 了一种综合季相和植被变化信息的不透水面提取框架.基于混合像元部分分解算法——混合调谐匹配滤波(MTMF),设计了多季相组合MTMF(SCMTMF)特征和多季相叠加MTMF(SSMTMF)两种策略,构造了不透水面的多季相MTMF特征,将不透水特征与多季相植被指数结合利用支持向量机实现对不透水面的精确分类.结果表明,利用多季相特征得到的不透水面提取效果相较于单季相有较明显的改善,该文所提出的策略有利于提高不透水面的估计精度.  相似文献   

地球-电离层空腔舒曼共振日变化特征分析     

银峰  张其林  纪彤彤  姜苏 《气象科学》2015,35(4):480-487

全球雷电活动在地球-电离层空腔中产生的极低频(ELF)信号干涉叠加,在一系列固定频率上产生舒曼共振(SR)。利用2012年5月以色列Mitzpe-Roman(MR)站ELF水平磁场资料,采用频谱变换、时间平均、分析了实测SR日变化信号的时域和频域特征。同时基于全球ELF传播模式,利用OTD/LIS雷电卫星资料模拟了5~30 Hz磁场功率谱日变化情况。结果表明:时域背景信号幅值的均值和偏差满足正态分布的期望和标准差;水平磁场前三阶SR谐振频率非常稳定,月平均下的谐振频率日变化相对8、14、20 Hz理论值的偏移量分别不超过0.3 Hz、0.55 Hz和0.6 Hz。东南亚和美洲地区雷电活动主要响应于南北磁场分量第一阶SR的07—09时和19—22时时段内。而东西磁场分量前三阶SR在12—15时时段内都对非洲地区雷电活动有指示作用。磁场功率谱日变化模拟结果与实测基本一致,表明利用单站正交磁天线的不同阶SR信号能够指示全球不同"热斑"区域的雷电活动。  相似文献   

Winding sense of galaxies around the local supercluster     

Binil Aryal 《中国天文和天体物理学报》2011,11(3)

We present an analysis of the winding sense(S and Z-shapes) of 1 621 field galaxies that have radial velocity between 3 000 km s-1 and 5 000 km s-1.The preferred alignments of S-and Z-shaped galaxies are studied using chi-square,autocorrelation and Fourier series tests.We classify all the galaxies into 32 subsamples and notice a good agreement between the position angle(PA) distribution of the S-and Zshaped galaxies.The homogeneous distribution of the S-and Z-shaped galaxies is more noticeable for the late-...  相似文献   

First photometric study of the eclipsing binary PS Persei     

Jin-Zhao Yuan 《中国天文和天体物理学报》2011,11(2)

CCD photometric observations of the eclipsing binary PS Persei (PS Per) were obtained on two consecutive days in 2009.The 2003 version of the WilsonDevinney code was used to analyze the first complete light curves in the V and R bands.It is found that PS Per is a short-period Algol-type binary with the less massive component completely filling its inner critical Roche lobe.The mass ratio of q=0.518 and the orbital inclination of i=89.86° are obtained.In addition,based on all available times of primary light...  相似文献   

Solar sail time-optimal interplanetary transfer trajectory design     

Sheng-Ping Gong  Yun-Feng Gao  Jun-Feng Li School of Aerospace  Tsinghua University  Beijing  China 《中国天文和天体物理学报》2011,(8)

The fuel consumption associated with some interplanetary transfer trajectories using chemical propulsion is not affordable. A solar sail is a method of propulsion that does not consume fuel. Transfer time is one of the most pressing problems of solar sail transfer trajectory design. This paper investigates the time-optimal interplanetary transfer trajectories to a circular orbit of given inclination and radius. The optimal control law is derived from the principle of maximization. An indirect method is used...  相似文献   

Photometric analysis of V30 of open cluster NGC 7789     

Yellapragada Ravi Kiron  Kandulapati Sriram  Pasagada Vivekananda Rao 《中国天文和天体物理学报》2011,(9)

We present the photometric solutions of the variable star V30 that is in the foreground of intermediate open cluster NGC 7789.The observations were done in the V passband using the 2 m telescope at the IUCAA-Girawali Observatory in India.The analysis is done using the Wilson-Devinney Code (2003) and the fitted light curve is presented.The photometric solutions reveal a W-subtype contact configuration.The photometric mass ratio is found to be 0.395 and the absolute masses and radii for the components are ded...  相似文献