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Title: Butterfly in a Cocoon, Understanding the Origin and Morphology of Globular Cluster Streams: The Case of GD-1

Journal Article · · The Astrophysical Journal (Online)

Tidally disrupted globular cluster (GC) streams are usually observed, and therefore perceived, as narrow, linear, and one-dimensional structures in the 6D phase space. In this paper, we show that the GD-1 stellar stream, which is the tidal debris of a disrupted GC, possesses a secondary diffuse and extended stellar component (~100 pc wide) around it, detected at the >5σ confidence level. Similar morphological properties are seen in synthetic streams that are produced from star clusters that are formed within dark matter sub-halos and then accrete onto a massive host galaxy. This lends credence to the idea that the progenitor of the highly retrograde GD-1 stream was originally formed outside of the Milky Way in a now defunct dark satellite galaxy. We deem that in future studies, this newly found cocoon component may serve as a structural hallmark to distinguish between the in situ and ex situ (accreted) formed GC streams.

Research Organization:
Univ. of Michigan, Ann Arbor, MI (United States)
Sponsoring Organization:
USDOE Office of Science (SC); Swedish Research Council (VR); Oskar Klein Centre for Cosmoparticle Physics; Leinweber Center for Theoretical Physics; National Aeronautics and Space Administration (NASA); National Development and Reform Commission; Alfred P. Sloan Foundation; National Science Foundation (NSF)
Grant/Contract Number:
SC0007859; 638-2013-8993; NNX15AK79G
OSTI ID:
1610970
Journal Information:
The Astrophysical Journal (Online), Vol. 881, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 29 works
Citation information provided by
Web of Science

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  • Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 474, Issue 2210 https://doi.org/10.1098/rspa.2017.0616
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Cited By (5)

Uncovering a 260 pc wide, 35-Myr-old filamentary relic of star formation journal November 2019
Exploring the Outskirts of Globular Clusters: The Peculiar Kinematics of NGC 3201 journal December 2019
The Density Structure of Simulated Stellar Streams journal January 2020
Phase-space Correlation in Stellar Streams of the Milky Way Halo: The Clash of Kshir and GD-1 journal November 2019
Exploring the outskirts of globular clusters: the peculiar kinematics of NGC 3201 text January 2019