中大學術數位典藏-NCU Institutional Repository-提供博碩士論文、考古題、期刊論文、研究計畫等下載:Item 987654321/102043
English  |  正體中文  |  简体中文  |  全文笔数/总笔数 : 94201/94201 (100%)
造访人次 : 81640600      在线人数 : 5421
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
搜寻范围 查询小技巧:
  • 您可在西文检索词汇前后加上"双引号",以获取较精准的检索结果
  • 若欲以作者姓名搜寻,建议至进阶搜寻限定作者字段,可获得较完整数据
  • 进阶搜寻


    jsp.display-item.identifier=請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/102043


    题名: ELLIPTICITIES of ELLIPTICAL GALAXIES in DIFFERENT ENVIRONMENTS
    作者: 高仲明;Chen, Cheng-Yu;Hwang, Chorng-Yuan;Ko, Chung-Ming
    贡献者: 理學院天文研究所
    关键词: Astrophysics;Density;Elliptical galaxies;Ellipticity;Filaments;Galactic clusters;Galactic evolution;galaxies: evolution;galaxies: formation;galaxies: fundamental parameters;Galaxy distribution;Sky surveys (astronomy);Space telescopes;Spatial distribution;Stars & galaxies
    日期: 2016-10-20
    上传时间: 2026-04-21 14:58:03 (UTC+8)
    出版者: IOP Publishing Ltd.;Philadelphia: The American Astronomical Society
    摘要: 摘要: ABSTRACT We studied the ellipticity distributions of elliptical galaxies in different environments. From the ninth data release of the Sloan Digital Sky Survey, we selected galaxies with absolute -band magnitudes between −21 and −22. We used the volume number densities of galaxies as the criterion for selecting the environments of the galaxies. Our samples were divided into three groups with different volume number densities. The ellipticity distributions of the elliptical galaxies differed considerably in these three groups of different density regions. We deprojected the observed 2D ellipticity distributions into intrinsic 3D shape distributions, and the result showed that the shapes of the elliptical galaxies were relatively spherically symmetric in the high density region (HDR) and that relatively more flat galaxies were present in the low density region (LDR). This suggests that the ellipticals in the HDRs and LDRs have different origins or that different mechanisms might be involved. The elliptical galaxies in the LDR are likely to have evolved from mergers in relatively anisotropic structures, such as filaments and webs, and might contain information on the anisotropic spatial distribution of their parent mergers. By contrast, elliptical galaxies in the HDR might be formed in more isotropic structures, such as galaxy clusters, or they might encounter more torqueing effects compared with galaxies in LDRs, thereby becoming rounder.
    其他題名: APJ
    其他題名: Astrophys. J
    出版者: Philadelphia: The American Astronomical Society
    出版日期: 2016-10-20
    出處: The Astrophysical journal, 2016-10, Vol.830 (2), p.123
    資源來源: Institute of Physics Journals
    版權: 2016. The American Astronomical Society. All rights reserved.
    版權: Copyright IOP Publishing Oct 20, 2016
    識別號: ISSN: 0004-637X
    識別號: ISSN: 1538-4357
    識別號: EISSN: 1538-4357
    識別號: DOI: 10.3847/0004-637X/830/2/123
    显示于类别:[天文研究所] 期刊論文

    文件中的档案:

    档案 描述 大小格式浏览次数
    index.html0KbHTML15检视/开启


    在NCUIR中所有的数据项都受到原著作权保护.

    社群 sharing

    ::: Copyright National Central University. | 國立中央大學圖書館版權所有 | 收藏本站 | 設為首頁 | 最佳瀏覽畫面: 1024*768 | 建站日期:8-24-2009 :::
    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - 隱私權政策聲明