2024
DOI: 10.3847/1538-4357/ad4299
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Slant, Fan, and Narrow: The Response of Stellar Streams to a Tilting Galactic Disk

Jacob Nibauer,
Ana Bonaca,
Mariangela Lisanti
et al.

Abstract: Stellar streams are sensitive tracers of the gravitational potential, which is typically assumed to be static in the inner Galaxy. However, massive mergers like Gaia-Sausage-Enceladus can impart torques on the stellar disk of the Milky Way that result in the disk tilting at rates of up to 10°–20° Gyr−1. Here, we demonstrate the effects of disk tilting on the morphology and kinematics of stellar streams. Through a series of numerical experiments, we find that streams with nearby apocenters (r … Show more

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“…GC orbits may also be affected by a variety of other factors not considered in this study, such as a time-dependent potential or changing disk orientation (e.g., Dillamore et al 2022;Nibauer et al 2024). Recent accretion of satellites is less likely to be important, since there have been no significant merger events in the inner Galaxy since the formation of the bar (Sanders et al 2024;Deason & Belokurov 2024).…”
Section: Discussionmentioning
confidence: 99%
“…GC orbits may also be affected by a variety of other factors not considered in this study, such as a time-dependent potential or changing disk orientation (e.g., Dillamore et al 2022;Nibauer et al 2024). Recent accretion of satellites is less likely to be important, since there have been no significant merger events in the inner Galaxy since the formation of the bar (Sanders et al 2024;Deason & Belokurov 2024).…”
Section: Discussionmentioning
confidence: 99%