巡洋 发表于 2025-3-21 16:56:32

书目名称Cold Gas at High Redshift影响因子(影响力)<br>        http://impactfactor.cn/if/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift影响因子(影响力)学科排名<br>        http://impactfactor.cn/ifr/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift网络公开度<br>        http://impactfactor.cn/at/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift网络公开度学科排名<br>        http://impactfactor.cn/atr/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift被引频次<br>        http://impactfactor.cn/tc/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift被引频次学科排名<br>        http://impactfactor.cn/tcr/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift年度引用<br>        http://impactfactor.cn/ii/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift年度引用学科排名<br>        http://impactfactor.cn/iir/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift读者反馈<br>        http://impactfactor.cn/5y/?ISSN=BK0229283<br><br>        <br><br>书目名称Cold Gas at High Redshift读者反馈学科排名<br>        http://impactfactor.cn/5yr/?ISSN=BK0229283<br><br>        <br><br>

宠爱 发表于 2025-3-21 22:28:07

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Vasoconstrictor 发表于 2025-3-22 01:15:37

The Neutral Hydrogen Distribution in Luminous Infrared Galaxiestwo spirals (Sanders .. 1988, Scoville .. 1991), it is somewhat surprising that the optical morphology of these systems differs from the classical double-tailed morphology of merging disks described by Toomre & Toomre (1972) and illustrated by the sequence of 11 disk-disk systems in progressively ad

才能 发表于 2025-3-22 08:02:26

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Hyperopia 发表于 2025-3-22 12:10:39

The Evolution of the Far-Infrared Galaxy Populationstarburst galaxy population and this is supported by the interpretation of the 60.m source-counts. The sub-mJy radio source population at 1.4 GHz has also been found to be essentially identical to the IRAS starburst galaxy population and faint radio source-counts support luminosity evolution models.

异端 发表于 2025-3-22 14:29:40

The European Large Area ISO Survey: Elaisbeing undertaken by ISO. The depth and areal coverage were designed to complement the various Guaranteed Time surveys. The main science thrust is to explore star formation in galaxies to a much higher redshift than was probed by IRAS. We expect to detect around 8000 extragalactic objects and a simil

异端 发表于 2025-3-22 18:49:26

Keck Observations of Microjansky Radio SourcesTo investigate their redshifts, star formation characteristics, optical morphologies, and evolution, we have used the 10-meter Keck telescope to obtain . broad-band images and optical spectra of a complete sample of .Jy sources detected in three fields at the VLA. In one field, only 1 of 16 sources

流利圆滑 发表于 2025-3-23 00:22:12

Small Scale Structure and High Redshift HId tunnels. Zel’dovich (1970) showed that gravitational instability in an expanding universe can create such structures from generic random initial conditions. Zeldovich’s analysis was originally used to describe the first collapse in “top-down” scenarios like the hot dark matter model, which have a

曲解 发表于 2025-3-23 02:38:40

Are the Lyman Alpha Forest “Clouds” Expanding Pancakes?structures of small overdensity. It is argued that the observed absorbers should be preferentially located in underdense regions of the universe and should typically expand faster than the Hubble flow.

自由职业者 发表于 2025-3-23 09:06:05

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查看完整版本: Titlebook: Cold Gas at High Redshift; Proceedings of a Wor M. N. Bremer,P. P. Werf,C. L. Carilli Conference proceedings 1996 Kluwer Academic Publisher