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Titlebook: Galaxy Evolution in Groups and Clusters; A JENAM 2002 Worksho Catarina Lobo,Margarida Serote Roos,Andrea Biviano Book 2003 Springer Science

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發(fā)表于 2025-3-21 19:18:16 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Galaxy Evolution in Groups and Clusters
副標(biāo)題A JENAM 2002 Worksho
編輯Catarina Lobo,Margarida Serote Roos,Andrea Biviano
視頻videohttp://file.papertrans.cn/381/380360/380360.mp4
圖書封面Titlebook: Galaxy Evolution in Groups and Clusters; A JENAM 2002 Worksho Catarina Lobo,Margarida Serote Roos,Andrea Biviano Book 2003 Springer Science
描述Galaxy groups and clusters provide excellent laboratories for studying galaxy properties in different environments and at different look-back times. In particular, the recent detections of high-redshift cluster candidates, only possible with the current high-technology instrumentation, add a new dimension to the problem. Along with the ever increasing computing power and sophisticated algorithms to model clusters of galaxies, it may help us to understand the origins of today‘s groups and clusters, as well as of their member galaxies. These workshop proceedings provide a snapshot of the current research in this subject, covering the observations, theory and numerical simulations relevant to galaxy evolution in groups and clusters. In this book, intended primarily to researchers in the field, particular emphasis is given to the recent impressive progress in the field, on important new results, and on the future prospects and open questions to be tackled.
出版日期Book 2003
關(guān)鍵詞Population; Redshift; Universe; X-ray; cluster; density; dispersion; environment; environmental effects; evol
版次1
doihttps://doi.org/10.1007/978-94-010-0107-6
isbn_softcover978-94-010-3975-8
isbn_ebook978-94-010-0107-6
copyrightSpringer Science+Business Media Dordrecht 2003
The information of publication is updating

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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:
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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.
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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.
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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
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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
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