Phase-space Correlation in Stellar Streams of the Milky Way Halo: The Clash of Kshir and GD-1

被引:22
|
作者
Malhan, Khyati [1 ]
Ibata, Rodrigo A. [2 ]
Carlberg, Raymond G. [3 ]
Bellazzini, Michele [4 ]
Famaey, Benoit [2 ]
Martin, Nicolas F. [2 ]
机构
[1] Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, AlbaNova, SE-10691 Stockholm, Sweden
[2] Univ Strasbourg, CNRS, Observ Astron Strasbourg, UMR 7550, F-67000 Strasbourg, France
[3] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada
[4] INAF Osservatorio Astrofis & Sci Spazio, Via Gobetti 93-3, I-40129 Bologna, Italy
基金
美国安德鲁·梅隆基金会; 美国国家科学基金会; 瑞典研究理事会;
关键词
GLOBULAR-CLUSTERS; DARK-MATTER; SAGITTARIUS; ORIGIN; FIELD; MAP;
D O I
10.3847/2041-8213/ab530e
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a <CDATA<i long stellar stream in the Milky Way halo, which criss-crosses the well known ?GD-1? stream. We show that this new stellar structure (?Kshir?) and GD-1 lie at similar distance, and are remarkably correlated in kinematics. We propose several explanations for the nature of this new structure and its possible association with GD-1. However, a scenario in which these two streams were accreted onto the Milky Way within the same dark matter sub-halo seems to provide a natural explanation for their phase-space entanglement, and other complexities of this coupled system.
引用
收藏
页数:7
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