退缩
发表于 2025-3-21 20:05:17
书目名称Dynamics and Interactions of Galaxies影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0283971<br><br> <br><br>书目名称Dynamics and Interactions of Galaxies读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0283971<br><br> <br><br>
Pert敏捷
发表于 2025-3-21 20:47:12
Are High Redshift Galaxies Interacting?rtunately, as far as mergers at high redshifts is concerned, I cannot bring myself to do this. Instead, I propose to present you with evidence that peculiar phenomena are occurring in the most distant galaxies we can study. According to your degree of faith in the “Book of Mergers”, you can decide w
衰老
发表于 2025-3-22 03:11:40
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DEFT
发表于 2025-3-22 05:20:24
Interactions in “Butcher-Oemler” Clusters of galaxies at redshifts near 0.4 contained a much larger population of “blue” galaxies than expected. This suggested rapid color evolution of galaxies in 1/3 of a Hubble time. In order to put this on a more quantitative level, Butcher and Oemler (1984a) undertook a photometric study of 33 clusters
Fantasy
发表于 2025-3-22 08:44:42
Are Our Globular Clusters Coeval?axy formed. A basic goal is to determine the time interval over which the Galactic halo and disk were formed, since a short time interval (< 1 Gyr) would be consistent with the picture of rapid, ordered collapse proposed by Eggen, Lynden-Bell, and Sandage (1962), whereas a much longer time interval
令人悲伤
发表于 2025-3-22 15:14:59
Stellar Populations and Mergerseach population being but a different stage in the process? Or have at least some of them nothing to do with the origins and evolution of the others, as expected from mergers? In the context of this meeting, we will look particularly at the latter possibility, and will discuss briefly the data suppo
令人悲伤
发表于 2025-3-22 21:06:11
A New Model of the Magellanic Stream of the Magellanic Stream. In contrast Zaritsky et al. (1989), using the statistical procedure developed by Little and Tremaine (1987), have found this mass to be 3.6 × 10. M. from the orbits of satellites of the Galaxy.
ABOUT
发表于 2025-3-23 00:47:23
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animated
发表于 2025-3-23 01:59:51
Status of Shell Galaxiesatalogue (Arp, 1966). But only recently has special attention has been drawn to them. The improvement of photographic emulsions, and the application of new photographic techniques such as “unsharp masking” and “contrast enhancement” by Malin (1977, 1981) has led to the discovery of shells and other
值得
发表于 2025-3-23 05:46:39
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