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1.
本文对ＩＲＡＳ暗源表中４个选区的ＩＲＡＳ星系的两点角相关函数，关联分维进行了计算，结果表明，所有选区内的星系呈现小角尺度上的成团，在较大角尺度上，分布可以用多级分形很好地表示，在更大角尺度上，用非归一星系对计数可以探测到密度分布中可能存在的典型惊讶，当取４个选区的平均值作为ＩＲＡＳ星系在宙宇中分布情况的代表时，所得结果与用全于ＩＲＡＳ点源表和其他巡天资料得到的结果一致。 相似文献
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本文对ＩＲＡＳ暗源表中４个选区内的ＩＲＡＳ星系的两点角相关函数，关联分维进行了计算。结果表明，所有选区内的星系呈现小角尺度上的成团。在较大角尺度上，分布可以用多级分形很好地表示。在更大角尺度上，用非归一星系对计数可以探测到密度分布中可能存在的典型尺度。当取４个选区的平均值作为ＩＲＡＳ星系在宇宙中分布情况的代表时，所得结果与用全天ＩＲＡＳ点源表和其他巡天资料得到的结果一致。 相似文献
3.
最近对哈勃常数的观测趋于一个大的值，引进宇宙学常数为主的宇宙学成了保持平坦宇宙并解决年龄矛盾的主要方法．本文讨论了（ｈ，Ω∧，ΩＭ）＝（０．８，０．８，０．２）的宇宙模型的一些后果，并和高红移椭球星系的观测，以及星系计数的观测作了比较．尽管观测事实表明Ω∧＝０．８模型比Ω∧＝０模型更具有优势，但这个结论仍是模糊的．除了年龄问题外，还不能排除（０．８，０，１）标准宇宙学的存在． 相似文献
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本文对两点相关函数及关联分维间的关系进行了讨论，以ＩＲＡＳ星系红移巡天样本作为例子进行分析，分析结果表明，在大尺度（≥１５─２０ｈＭｐｃ）上，ＩＲＡＳ星系的分布既不能用简单幂律形式的两点相关函数，也不能用简单分形来描写。它可以用多级分形来更好地描写。多级分形结构的主要特征之一是存在典型尺度，即相邻分形级间的转变尺度，用非归一计数方法可以有效而准确地确定这些典型尺度，存在典型尺度对目前已有的结构形成模型提出了挑战。 相似文献
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本文对具有初始几何形状及维里系数相同,但初始速度弥散度分布不同的三轴椭球进行了数值模拟。四个模型的最后质点分布及等密度轮廓的图象表明,三轴椭球的塌缩是与初始弥散速度的分布密切相关的。而不同的初始弥散速度分布可能与原星系在薄饼中不同的碎裂时刻有关。 相似文献
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具有哈勃流的相对论抛射运动学(II)15个超光速源解的应用 总被引：1，自引：0，他引：1
龚树模 《中国天文和天体物理学报》1997,(4)
研究超光速运动的要点是求出正喷流和反喷流的多普勒因子．在传统方法中，反喷流的方向取为正喷流的反方向，其流速相等．正确的方法是先从由局部抛射和哈勃流组成的正喷流中，用狭义相对论的合速公式分解出局部抛射速度，然后从哈勃流和反方向的局部抛射速度导出反喷流的速度和方向．这就是本文所求出的结果．本文的主要目的是比较用传统方法和本文方法所得的反喷流的多普勒因子的值．最后解得１５个超光速源，其结果显示传统方法所得的反喷流多普勒因子的值，除以红移ｚ的函数，ｆ（ｚ）＝１．０１０ｚ２＋１．９９２ｚ＋０．９９３，就得到本文所得的反喷流多普勒因子的值；在ｚ＝０．０５６９－２．３６７范围内，上式的标准误差为０００８２８．应用本文方法，若有足够多的超光速和亚光速源的数据，有可能提供测定哈勃常数Ｈ０和在活动类星体中寻找蓝移吸收线． 相似文献
8.
景益鹏 《中国天文和天体物理学报》1989,(1)
本文对D≤4,R≥0的Abell团样品和整个R≥3的Abell团样品的空间两点相关函数做了统计分析,结果表明R≥0,R=0和R≥3的Abell团的相关函数分别为175r~(-1.8),150r~(-1.8)和1900r~(-1.8)利用已有的R≥1和R≥2团的相关函数的统计结果,我们得到了Abell团的相关性幅度α与富度N之间的关系:α∝N~(1.6)。在相关性幅度的统计误差所允许的范围内,α与N之间的关系可以在宇宙弦理论中得到解释。 相似文献
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两点相关函数,关联分维及IRAS星系大尺度分布的典型尺度 总被引：1，自引：1，他引：0
本对两点相关函数及关联分维间的关系进行了讨论，以ＩＲＡＳ星系红移天样本作为例子进行分析。分析结果表明，在大尺度上，ＩＲＡＳ星系的分布既不能用简单幂律形式的两点关函数，也不能用简单分形来描写，它可以用多级分形来更好地描写，多级分形结构的主要特征之一是存在典型尺度，即相邻分形间的转变尺度，用非归一计数方法可以有效耐 准确地确定这些典型尺度。存在典型尺度对目前已有的结构形成模型提出了挑战。 相似文献
10.
本文在Wen等人工作的基础上,对CfA红移巡天样本中银道以北和以南天区中星系的大尺度分布分别进行了分维计算并比较其所得结果。分析表明,这两个区域内星系的大尺度分布存在显著差异。说明CfA样本还不能构成代表宇宙大尺度结构的好样本。另一方面,两个区域中样本分析结果又存在着一些明显的共同点:它们都表现出明显的多级分形特征。结合对IRAS星系红移巡天样本和星系分立小天区红移巡天样本的分析结果。我们认为,多级分形很可能是宇宙大尺度结构的一个普遍和重要的特征。本文对这一特征的含义也作了简略的讨论。 相似文献
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Abstract— The relative abundance of different compositional types and mass frequency distributions are presented for four meteorite samples (the modern falls, Antarctic finds, Yamato finds and Allan Hills Main Icefield finds). The modern falls sample represents continuous collection of a known number of falls over a short timespan, while the Antarctic samples represent a longer timespan and an unknown number of falls. The Allan Hills Main Icefield sample has many desirable collection characteristics indicating it best represents Antarctic meteorites. By retabulating the modern falls to create a sample with characteristics similar to those of the Allan Hills Main Icefield finds, we can directly compare the two. The mass frequency distributions of Antarctic samples exhibit a tail toward the larger sizes and thus differ from that of the modern falls (which approximates a normal curve). In general, normal and power law models prove to be inadequate to explain the observed mass frequency distributions, possibly because they fail to correctly account for atmospheric and collection effects. Non-parametric statistics show that it is unlikely that the two are good samples of a single steady-state meteoritic complex. In addition, there is an excess in numbers of small H chondrites in Allan Hills Main Icefield finds relative to modern falls which is not easy to explain given modern showerfall rates of occurrence. This supports the view that the delivery of meteoritic material to Earth might be variable over the short timescale represented by these samples. 相似文献
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D. W. E. Green 《Astronomische Nachrichten》2004,325(9):689-701
Contemporary European measurements of the Milky Way supernova of 1572 (B Cas) have been analyzed to compute a modern position for the star in 1572. This work adds to that done by previous 20th‐century authors by using a new procedure and previously unused astrometry by 16th‐century European observers. Comparison is made with earlier analyses and to modern positional data on the supernova remnant (3C 10). (© 2004 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
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The effect of vegetation on the Younger Dryas (YD) climate is studied by comparing the results of four experiments performed with the ECHAM-4 atmospheric general circulation model (AGCM): (1) modern control climate, (2) simulation with YD boundary conditions, but with modern vegetation, (3 and 4) identical to (2), but with paleo-vegetation. Prescribing paleo-vegetation instead of modern vegetation resulted in temperature anomalies (both positive and negative) of up to 4°C in the Northern Hemisphere mid-latitudes, mainly as an effect of changes in forest cover (change in albedo). Moreover, changes in precipitation and evaporation were found, most notably during December–January–February (DJF) in the tropics and were caused by the replacement of forests by grasslands. These results are consistent with other model studies on the role of vegetation changes on climate and they suggest that it is important in paleoclimate simulation studies to prescribe realistic vegetation types, belonging to the period of interest. However, in our case the addition of YD vegetation did not improve the agreement with proxy data in Europe, as the temperatures were increasing during winter compared to the YD simulation with modern vegetation. It must be noted that this increase was not statistically significant. The model-data mismatch suggests that other factors probably played an important role, such as permafrost and atmospheric dust. We infer that during the last glacial-interglacial transition, the time lag between the first temperature increase and the northward migration of trees, estimated at 500–1000 years, could have delayed the warming of the Eurasian continent. The relatively open vegetation that existed during the early stages of the last glacial-interglacial transition had a relatively high albedo, thus tempering warming up of the Eurasian land surfaces. 相似文献
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Brian Warner 《Astrophysics and Space Science》1995,230(1-2):1-7
A brief overview is given of the history of astrophysics in South Africa up to the beginning of the modern era. 相似文献
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现代科学表明宇宙中99%以上的可观测物质都处于等离子体状态,从小尺度的微观粒子动力学集体过程与能量转换机制到大尺度的宇宙等离子天体结构状态与爆发活动现象,都是等离子天体物理学的研究课题.从宇宙演化历史、大尺度结构形成以及爆发活动现象等方面,系统地论述了等离子天体物理学在现代天文学发展以及现代等离子体宇宙观形成中的重要作用.同时,结合空间卫星科学探测研究及其对现代天文学的巨大影响,进一步阐述了地球磁层和日球层等空间等离子体实地探测研究在等离子天体物理学研究中所扮演的“天然实验室”的独特作用. 相似文献
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Recent technical progress of solar radio spectrography is concerned with digital data recording, the achievement of high time and frequency resolution, and with an improved coverage of the radio range at short and long wavelengths. A spatially-distributed network of radio spectrographs allows for complementary information about solar events and periods of activity selected for detailed investigation.By modern radio spectrographs a wealth of not yet adequately classified spectral fine structures can be observed, some of them potentially intimately related to effects of fragmentation of flare energy and/or to processes related to coronal heating. Requirements for the choice of technical parameters of solar spectrographs for checking theoretical models of fundamental processes of energy release are reflected in modern instruments. Prospects for future observations are briefly included. 相似文献
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Dmitri A. Uzdensky 《Astrophysics and Space Science》2004,292(1-4):573-585
In this review I consider modern theoretical models of coupled star–disk magnetospheres. I discuss a number of models, both stationary and time-dependent, and examine what physical conditions govern the selection of a preferred model. 相似文献
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Acid saline lake systems in Western Australia may be the best known modern terrestrial analog for the Burns formation on Mars and, thus, provide information about past environments and life on Mars. 相似文献
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Luiz Paulo R. Vaz 《Astrophysics and Space Science》1985,113(2):349-364
The weakest point in the modern models of eclipsing binary systems (EBS) is the treatment given to the effects of mutual irradiation. In this review, which does not have a similar one in the literature, I tried to collect all the work done on the irradiation problem until the middle of 1984, in order to make possible an evaluation of the present status of problem. Special emphasis is given to the applicability of the results to the analysis of EBS. The treatment given to the effect by the early studies as well as by practically all the modern models of EBS is described, and special attention is given to works analysing the problem using stellar model atmospheres. It turns out that the effect is more complex than suspected earlier, but that significant progress has been made recently.Review article. 相似文献