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The Ophiuchus stream progenitor: a new type of globular cluster and its possible Sagittarius connection

Lane, James MM; Navarro, Julio F; Fattahi, Azadeh; Oman, Kyle A; Bovy, Jo

The Ophiuchus stream progenitor: a new type of globular cluster and its possible Sagittarius connection Thumbnail


Authors

James MM Lane

Julio F Navarro

Kyle A Oman

Jo Bovy



Abstract

The Ophiuchus stream is a short arc-like stellar feature of uncertain origin located ∼5 kpc North of the Galactic centre. New proper motions from the second Gaia data release reconcile the direction of motion of stream members with the stream arc, resolving a puzzling mismatch reported in earlier work. We use N-body simulations to show that the stream is likely only on its second pericentric passage, and thus was formed recently. The simulations suggest that most of the disrupted progenitor is visible in the observed stream today, and that little further tidal debris is expected to lie beyond the ends of the stream. The luminosity, length, width, and velocity dispersion of the stream suggest a globular cluster (GC) progenitor substantially fainter and of lower surface brightness than estimated in previous work, and unlike any other known globulars in the Galaxy. This result suggests the existence of clusters that would extend the known GC population to fainter and more weakly bound systems than hitherto known. How such a weakly bound cluster of old stars survived until it was disrupted so recently, however, remains a mystery. Integrating backwards in time, we find that the orbits of Sagittarius and Ophiuchus passed within ∼5 kpc of each other about ∼100 Myr ago, an interaction that might help resolve this puzzle.

Citation

Lane, J. M., Navarro, J. F., Fattahi, A., Oman, K. A., & Bovy, J. (2020). The Ophiuchus stream progenitor: a new type of globular cluster and its possible Sagittarius connection. Monthly Notices of the Royal Astronomical Society, 492(3), 4164-4174. https://doi.org/10.1093/mnras/staa095

Journal Article Type Article
Acceptance Date Dec 30, 2019
Online Publication Date Jan 14, 2020
Publication Date Mar 31, 2020
Deposit Date Mar 25, 2020
Publicly Available Date Mar 28, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 492
Issue 3
Pages 4164-4174
DOI https://doi.org/10.1093/mnras/staa095

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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s) . Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.





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