Searching for the GD-1 stream progenitor in Gaia DR2 with direct N-body simulations
Abstract
We perform a large suite of direct N-body simulations aimed at revealing the location of the progenitor, or its remnant, of the GD-1 stream. Data from Gaia DR2 reveal that the GD-1 stream extends over ≈100°, allowing us to determine the stream's leading and trailing ends. Our models suggest that the length of the stream is consistent with a dynamical age between 2 and 3 Gyr and the exact length, width, and location of the GD-1 stream correspond to the stream's progenitor being located between -30° < ϕ1, pro < -45° in the standard GD-1 coordinate system. The model stream density profiles reveal that intact progenitors leave a strong overdensity, recently dissolved progenitors appear as gaps in the stream as escaped stars continue to move away from the remnant progenitor's location, and long-dissolved progenitors leave no observational signature on the remaining stream. Comparing our models to the GD-1 stream yields two possible scenarios for its progenitor's history: (a) the progenitor reached dissolution approximately 500 Myr ago during the cluster's previous perigalactic pass and is both located at and responsible for the observed gap at ϕ1 = -40° or (b) the progenitor reached dissolution over 2.5 Gyr ago, the fully dissolved remnant is at -30° < ϕ1 < -45°, and an observational signature of its location no longer exists. That the dissolved progenitor is in the range -30° < ϕ1 < -45° implies that density fluctuations outside of this range, e.g. a deep gap at ϕ1 ≈ -20°, are likely produced by compact baryonic or dark-matter perturbers.
- Publication:
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Monthly Notices of the Royal Astronomical Society
- Pub Date:
- June 2019
- DOI:
- arXiv:
- arXiv:1811.07022
- Bibcode:
- 2019MNRAS.485.5929W
- Keywords:
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- galaxies: star clusters: general;
- galaxies: structure;
- cosmology: dark matter;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 9 pages, 5 figures, Accepted for publication in MNRAS