不要提吃饭
发表于 2025-3-21 19:18:16
书目名称Galaxy Evolution in Groups and Clusters影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0380360<br><br> <br><br>书目名称Galaxy Evolution in Groups and Clusters读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0380360<br><br> <br><br>
chondromalacia
发表于 2025-3-21 23:41:11
Quantitative Study of Galaxy Morphology Release (SDSS EDR) galaxies of known redshift and brighter than r=16. The bulge-to-disk (B/D) luminosity ratios can be combined with an estimate of the galaxy’s local environment to address a number of key issues that are central to our understanding of galaxy formation:
subacute
发表于 2025-3-22 00:23:51
Characteristics of Meat Demand in GreeceWe derive the blue fraction for a sample of . -selected galaxies in 25 clusters at 0.15 < . < 0.92. We find a much smaller blue fraction and weaker trend with redshift than measured in optically selected samples. We suggest that the Butcher-Oemler effect is primarily due to star fonning low luminosity galaxies.
–DOX
发表于 2025-3-22 07:10:35
The , -Selected Butcher-Oemler EffectWe derive the blue fraction for a sample of . -selected galaxies in 25 clusters at 0.15 < . < 0.92. We find a much smaller blue fraction and weaker trend with redshift than measured in optically selected samples. We suggest that the Butcher-Oemler effect is primarily due to star fonning low luminosity galaxies.
使厌恶
发表于 2025-3-22 12:33:29
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diathermy
发表于 2025-3-22 16:58:17
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diathermy
发表于 2025-3-22 20:14:27
An Object Model for Geologic Map Informationlaxy evolution. This review discusses some of the recent observations of moderate to high redshift clusters. A consistent picture of galaxy evolution in clusters appears to be emerging, which includes a population of galaxies which formed early in the cluster history, as well as field galaxies which
amputation
发表于 2025-3-23 01:03:15
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Spinal-Tap
发表于 2025-3-23 03:33:06
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Basilar-Artery
发表于 2025-3-23 07:26:13
James A. Rodger,James A. Georgethe Nearby Optical Galaxy sample, by means of hierarchical and percolation ‘friends-of-friends’ methods. We find that earlier-type (brighter) galaxies are more clustered and lie closer to the group centers, both in position and in velocity, than later-type (fainter) galaxies. Spatial segregations ar