Flipping of the Tidal Tails of the Ophiuchus Stream due to the Decelerating Galactic Bar

Flipping of the Tidal Tails of the Ophiuchus Stream due to the Decelerating Galactic Bar

The Ophiuchus stellar stream presents a puzzle due to its complicated morphology, with a substructure perpendicular to the main track (spur), a broadened tail (fanning), and a shorter than expected angular extent given its old stellar population and short orbital period. The location of the stream a...

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Bibliographic Details
Main Authors: Yong Yang, Geraint F. Lewis, Denis Erkal, Ting S. Li, Andrew P. Li, Sarah L. Martell, Lara R. Cullinane, Guilherme Limberg, Daniel B. Zucker, Joss Bland-Hawthorn, Andrew B. Pace, Gary S. Da Costa, Alexander P. Ji, Sergey E. Koposov, Kyler Kuehn, Nora Shipp, Miles Pearson, Sam A. Usman, S5 Collaboration
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Stellar streams
Globular star clusters
Galactic bar
Milky Way Galaxy
Stellar dynamics
Milky Way dynamics
Online Access:https://doi.org/10.3847/1538-4357/adc57c
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https://doi.org/10.3847/1538-4357/adc57c

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