High-resolution N-body simulations of galactic cannibalism:: The Magellanic Stream

被引：16

作者：

Connors, TW ^{[1
]}

Kawata, D ^{[1
]}

Maddison, ST ^{[1
]}

Gibson, BK ^{[1
]}

机构：

[1] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 2004年 / 21卷 / 02期

关键词：

methods : N-body simulations; galaxies : interactions; Magellanic Clouds;

D O I：

10.1071/AS04014

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Hierarchical clustering represents the favoured paradigm for galaxy formation throughout the Universe; due to its proximity, the Magellanic system offers one of the few opportunities for astrophysicists to decompose the full six-dimensional phase-space history of a satellite in the midst of being cannibalised by its host galaxy. The availability of improved observational data for the Magellanic Stream and parallel advances in computational power has led us to revisit the canonical tidal model describing the disruption of the Small Magellanic Cloud and the consequent formation of the Stream. We suggest improvements to the tidal model in light of these recent advances.

引用

页码：222 / 227

页数：6

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Istituto dei Sistemi Complessi Consiglio Nazionale delle Ricerche, Via dei Taurini 19, Rome
00185, Italy
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F-75005, France
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F-75005, France
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00184, Italy
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