Flipping of the tidal tails of the Ophiuchus stream due to the decelerating Galactic bar
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| Format: | Preprint |
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2025
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| author | Yang, Yong Lewis, Geraint F. Erkal, Denis Li, Ting S. Li, Andrew P. Martell, Sarah L. Cullinane, Lara R. Limberg, Guilherme Zucker, Daniel B. Bland-Hawthorn, Joss Pace, Andrew B. Da Costa, Gary S. Ji, Alexander P. Koposov, Sergey E. Kuehn, Kyler Shipp, Nora Pearson, Miles Usman, Sam A. Collaboration, S5 |
| author_facet | Yang, Yong Lewis, Geraint F. Erkal, Denis Li, Ting S. Li, Andrew P. Martell, Sarah L. Cullinane, Lara R. Limberg, Guilherme Zucker, Daniel B. Bland-Hawthorn, Joss Pace, Andrew B. Da Costa, Gary S. Ji, Alexander P. Koposov, Sergey E. Kuehn, Kyler Shipp, Nora Pearson, Miles Usman, Sam A. Collaboration, S5 |
| contents | 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 approaches the Galactic center, implying a possible connection between its orbit and its unusual morphology. Here we demonstrate that the morphology of Ophiuchus can be attributed to its interaction with the decelerating Galactic bar, which leads to the flipping or transposition of its tidal tails. The short length of the stream is the result of stars stripped in the ancient past still remaining concentrated, and the spur, as well as the fanning, are composed of either leading or trailing tails built up of stars released at different time intervals. Our new spectroscopic data, obtained as part of the Southern Stellar Stream Spectroscopic Survey $(S^5)$, and modeling of Ophiuchus indicate that, in the presence of the bar, an initial leading tail can be redistributed to the trailing side and vice versa, and the morphology of a stream can be reshaped. This result confirms that the Galactic bar plays a vital role in reconstructing the orbital behavior of streams passing close to the central region of the Milky Way. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2503_19221 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Flipping of the tidal tails of the Ophiuchus stream due to the decelerating Galactic bar Yang, Yong Lewis, Geraint F. Erkal, Denis Li, Ting S. Li, Andrew P. Martell, Sarah L. Cullinane, Lara R. Limberg, Guilherme Zucker, Daniel B. Bland-Hawthorn, Joss Pace, Andrew B. Da Costa, Gary S. Ji, Alexander P. Koposov, Sergey E. Kuehn, Kyler Shipp, Nora Pearson, Miles Usman, Sam A. Collaboration, S5 Astrophysics of Galaxies 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 approaches the Galactic center, implying a possible connection between its orbit and its unusual morphology. Here we demonstrate that the morphology of Ophiuchus can be attributed to its interaction with the decelerating Galactic bar, which leads to the flipping or transposition of its tidal tails. The short length of the stream is the result of stars stripped in the ancient past still remaining concentrated, and the spur, as well as the fanning, are composed of either leading or trailing tails built up of stars released at different time intervals. Our new spectroscopic data, obtained as part of the Southern Stellar Stream Spectroscopic Survey $(S^5)$, and modeling of Ophiuchus indicate that, in the presence of the bar, an initial leading tail can be redistributed to the trailing side and vice versa, and the morphology of a stream can be reshaped. This result confirms that the Galactic bar plays a vital role in reconstructing the orbital behavior of streams passing close to the central region of the Milky Way. |
| title | Flipping of the tidal tails of the Ophiuchus stream due to the decelerating Galactic bar |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2503.19221 |