找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

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

[復制鏈接]
樓主: T-cell
51#
發(fā)表于 2025-3-30 09:49:00 | 只看該作者
https://doi.org/10.1007/978-3-8351-9227-0 A concentration of galaxies, apparently coincident with 2151–5805 on the sky, is found to lie in the background at a higher redshift, illustrating how the knowledge of redshifts can resolve structure in three dimensions. Much faster and more objective automatic methods of determining the redshifts are currently being developed.
52#
發(fā)表于 2025-3-30 12:26:00 | 只看該作者
53#
發(fā)表于 2025-3-30 17:03:32 | 只看該作者
54#
發(fā)表于 2025-3-31 00:46:07 | 只看該作者
The Spatial and Peculiar Velocity Distribution of Galaxies within 80 MPC,vertically through Figure 1. The other empty zone is caused by the gap in the catalogues between declinations ?17°.5 to ?2°.5. The 2-dimensional distribution in Figure 1 gives a strong visual impression of filamentary structure on angular scales up to a radian and more.
55#
發(fā)表于 2025-3-31 03:58:46 | 只看該作者
56#
發(fā)表于 2025-3-31 07:16:51 | 只看該作者
Kurt Magnus,Karl Popp,Walter Sextronly composed of spirals. The possible connection of a cloud of galaxies surrounding the cluster A569, the new filament in Gemini and the Linx-Ursa Major supercluster with the Perseus supercluster is briefly discussed.
57#
發(fā)表于 2025-3-31 09:15:33 | 只看該作者
A Redshift Survey in the Linx Gemini Region,nly composed of spirals. The possible connection of a cloud of galaxies surrounding the cluster A569, the new filament in Gemini and the Linx-Ursa Major supercluster with the Perseus supercluster is briefly discussed.
58#
發(fā)表于 2025-3-31 15:17:17 | 只看該作者
Superclusters,dimensions ranging from tens of kiloparsecs to hundreds of Megaparsecs. The rich clusters may be the largest bound structures. The superclusters look largely unrelaxed: they have rarely a well-defined centre; their relatively small internal random motions indicate crossing times along the larger dia
59#
發(fā)表于 2025-3-31 21:12:20 | 只看該作者
60#
發(fā)表于 2025-3-31 21:55:58 | 只看該作者
 關于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-10 23:40
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權所有 All rights reserved
快速回復 返回頂部 返回列表
奇台县| 海南省| 吴旗县| 景谷| 宜兰县| 霸州市| 滕州市| 岑溪市| 兰考县| 茂名市| 临漳县| 延边| 昂仁县| 牡丹江市| 苗栗市| 永新县| 唐海县| 遂宁市| 北京市| 化隆| 海安县| 察雅县| 高青县| 邹平县| 西城区| 正定县| 绥化市| 江门市| 隆回县| 张家川| 景东| 庆城县| 汾阳市| 平邑县| 汝州市| 沅江市| 洪雅县| 元谋县| 商南县| 新平| 都兰县|