Infall of substructures onto a Milky Way-like dark halo.pdf

Infall of substructures onto a Milky Way-like dark halo.pdf

  1. 1、本文档共9页,可阅读全部内容。
  2. 2、有哪些信誉好的足球投注网站(book118)网站文档一经付费(服务费),不意味着购买了该文档的版权,仅供个人/单位学习、研究之用,不得用于商业用途,未经授权,严禁复制、发行、汇编、翻译或者网络传播等,侵权必究。
  3. 3、本站所有内容均由合作方或网友上传,本站不对文档的完整性、权威性及其观点立场正确性做任何保证或承诺!文档内容仅供研究参考,付费前请自行鉴别。如您付费,意味着您自己接受本站规则且自行承担风险,本站不退款、不进行额外附加服务;查看《如何避免下载的几个坑》。如果您已付费下载过本站文档,您可以点击 这里二次下载
  4. 4、如文档侵犯商业秘密、侵犯著作权、侵犯人身权等,请点击“版权申诉”(推荐),也可以打举报电话:400-050-0827(电话支持时间:9:00-18:30)。
查看更多
Infall of substructures onto a Milky Way-like dark halo

Mon. Not. R. Astron. Soc. 000, 1–9 (2007) Printed 11 March 2008 (MN LATEX style file v2.2) Infall of Substructures onto a Milky Way-like Dark Halo Yang-Shyang Li? and Amina Helmi? Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700 AV Groningen, The Netherlands 11 March 2008 ABSTRACT We analyse the dynamical properties of substructures in a high-resolution dark matter simu- lation of the formation of a Milky Way-like halo in a ΛCDM cosmology. Our goal is to shed light on the dynamical peculiarities of the Milky Way satellites. Our simulations show that about 1/3 of the subhalos have been accreted in groups. We quantify this clustering by mea- suring the alignment of the angular momentum of subhalos in a group. We find that this signal is visible even for objects accreted up to z ~ 1, i.e. 8 Gyr ago, and long after the spatial coher- ence of the groups has been lost due the host tidal field. This group infall may well explain the ghostly streams proposed by Lynden-Bell Lynden-Bell to orbit the Milky Way. Our analy- ses also show that if most satellites originate in a few groups, the disk-like distribution of the Milky Way satellites would be almost inevitable. This non-random assignment of satellites to subhalos implies an environmental dependence on whether these low-mass objects are able to form stars, possibly related to the nature of reionization in the early Universe. With this picture, both the “ghostly streams” and the “disk-like configuration” are manifestations of the same phenomenon: the hierarchical growth of structure down to the smallest scales. Key words: methods: numerical - Galaxy: formation - galaxies: dwarf - galaxies: kinematics and dynamics - dark matter. 1 INTRODUCTION In cold dark-matter (CDM) cosmologies, large galaxies are the re- sult of the aggregation of smaller subunits. Some of these subunits may survive until the present day in the form of satellites, while some may be completely destroyed in the course of time,

文档评论(0)

l215322 + 关注
实名认证
内容提供者

该用户很懒,什么也没介绍

1亿VIP精品文档

相关文档