Titlebook: Clusters and Groups of Galaxies; International Meetin F. Mardirossian,G. Giuricin,M. Mezzetti Book 1984 D. Reidel Publishing Company, Dordr

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書目名稱Clusters and Groups of Galaxies影響因子(影響力)




書目名稱Clusters and Groups of Galaxies影響因子(影響力)學(xué)科排名




書目名稱Clusters and Groups of Galaxies網(wǎng)絡(luò)公開度




書目名稱Clusters and Groups of Galaxies網(wǎng)絡(luò)公開度學(xué)科排名




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書目名稱Clusters and Groups of Galaxies讀者反饋




書目名稱Clusters and Groups of Galaxies讀者反饋學(xué)科排名

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https://doi.org/10.1007/978-3-8351-9227-0prism plates using the COSMOS plate-scanning machine. 2294 redshifts have been measured in a 4.7 × 5.2 deg area of the sky which includes part of the Indus supercluster. The redshifts enable the three-dimensional distribution of the galaxies within the supercluster to be investigated, and a subset o

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Grundbegriffe und Darstellungsmittel,n the northern hemisphere. It will be some years before the quantity and quality of redshifts in the southern hemisphere can complement the northern data and correct the imbalance. In the meantime, we wish to offer a preliminary examination using available data — albeit somewhat heterogeneous.

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Grundbegriffe und Darstellungsmittel,lumes of space (e.g. Davis .. 1981; Gregory and Thompson 1978). These surveys have been important in identifying the existence and measuring the sizes of superclusters and voids. However, one must sample much larger volumes to truly map out the three dimensional structure of matter and to differenti

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