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Reginald Sutcliffe and the Invention of Modern Weather Systems Science最新文献

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Background 背景
Pub Date : 2001-01-01 DOI: 10.18356/cc3fe502-en
W. Sokolowski
This report provides an overview of research into high redshift galaxies and galaxy evolution from an ob servational perspective over the period 1990 to 1993. Only references to the literature from this period are given in order to provide a snapshot of current research. Several related topics (e.g. high-redshift galaxies as probes of cosmological models, galaxy interactions and evolution at low redshift, and gravitational lensing) are dealt with elsewhere in this volume. clusters. A second sizable catalogue of high-redshift clusters appeared 25 , while several groups investigated the high fraction of blue galaxies in distant clusters (the Butcher-Oemler effect), both through photometric studies 87 and spectroscopically 36,37 . These studies confirmed the strong increase in the blue fraction with redshift and demonstrated that it is largely composed of emission-line and E+A galaxies that are much scarcer in clusters selection biases with the in rich to the all have a large blue fraction at high redshift, with the richer groups redder at low redshift. is also 36,2 for of the in with z=0.5-l, with as as present-day ellipticals by zssl. Ly a absorbers have been discovered through their Ly a, [Oil], H/J or CO , and appear consistent with large star-forming disks. Recent observations suggest that the clustering of Ly a-emitting galaxies around Ly a absorbers, and of the absorbers themselves, is strong over scales of several Mpc, in contrast to the weak clustering of faint galaxies 108,48 the limit (LL) and metal line (Mgll and CIV) absorbers on scales decrease the of (clouds) at larger impact equivalent width of the Mgll systems decreases with time , implying a decrease in the the number of clouds per . The Mgll and CIV systems are also clustered 84,100 on scales of several Mpc. QSO of dark in
本报告从观测的角度概述了1990年至1993年期间高红移星系和星系演化的研究。仅参考这一时期的文献,以便提供当前研究的快照。几个相关的主题(例如高红移星系作为宇宙模型的探测器,星系在低红移的相互作用和演化,以及引力透镜)在本卷的其他地方处理。集群。第二份相当大的高红移星系团的目录出现了(25),同时有几个小组通过光度研究(87)和光谱学(36,37)研究了遥远星系团中蓝色星系的高比例(布彻-欧姆勒效应)。这些研究证实了随着红移蓝色部分的强烈增加,并证明它主要由发射线和E+A星系组成,这些星系在星团选择偏差中要少得多,在高红移时,它们都有很大的蓝色部分,而在低红移时,更富的星团更红。在z=0.5-l的椭圆中,也有36,2个与现在的椭圆相同。通过它们的Ly a, [Oil], H/J或CO发现了Ly a吸收体,并且看起来与大型恒星形成盘一致。最近的观测表明,在几个Mpc尺度上,发射Ly a的星系在Ly a吸收体周围以及吸收体本身的聚集是强烈的,与微弱星系的弱聚集相反,在较大的撞击下,尺度上的极限(LL)和金属线(Mgll和CIV)吸收体减少(云),Mgll系统的等效宽度随着时间的推移而减少,这意味着每个云的数量减少。mll和CIV系统也以几个Mpc的规模聚集在一起。暗的QSO
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引用次数: 0
An Active Retirement 积极退休
Pub Date : 1993-03-01 DOI: 10.7748/NOP.5.2.46.S40
A. Hull
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引用次数: 0
Director of Research and the Development of Numerical Weather Prediction 数值天气预报研究及发展主任
Pub Date : 1900-01-01 DOI: 10.2307/j.ctv16km22z.11
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引用次数: 0
The Emergence of an International Figure 一个国际人物的出现
Pub Date : 1900-01-01 DOI: 10.2307/j.ctv16km22z.13
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引用次数: 0
Homecoming and the Development Theorem 返乡与发展定理
Pub Date : 1900-01-01 DOI: 10.2307/j.ctv16km22z.10
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引用次数: 0
Reflection and Twilight 倒影与黄昏
Pub Date : 1900-01-01 DOI: 10.2307/j.ctv16km22z.16
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引用次数: 0
[Illustrations] (插图)
Pub Date : 1900-01-01 DOI: 10.2307/j.ctv16km22z.12
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引用次数: 0
An Unexpected Career: 意想不到的职业:
Pub Date : 1900-01-01 DOI: 10.2307/j.ctv16km22z.7
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引用次数: 7
Professor Sutcliffe: 拍摄的教授:
Pub Date : 1900-01-01 DOI: 10.2307/j.ctv16km22z.14
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引用次数: 0
The War Years: 战争年代:
Pub Date : 1900-01-01 DOI: 10.1007/978-1-349-18723-2_8
A. Davies
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引用次数: 0
期刊
Reginald Sutcliffe and the Invention of Modern Weather Systems Science
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