C-19 and Hot, Wide Star Streams

The C-19 star stream has the abundance characteristics of an unusually metal-poor globular cluster but kinematically is uncharacteristically hot and wide for a cluster stream, having a line-of-sight velocity dispersion of 7  ±  2 km s ^−1 and a 1 σ width of 240 pc. We show that the tidal dissolution...

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Bibliographic Details
Main Authors: Raymond G. Carlberg, Rodrigo Ibata, Nicolas F. Martin, Else Starkenburg, David S. Aguado, Khyati Malhan, Kim Venn, Zhen Yuan
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ade4ce
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