Icarus: a Flat and Fast Prograde Stellar Stream in the Milky Way disk

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Paola Re Fiorentin, Alessandro Spagna, Mario G. Lattanzi, Michele Cignoni

We explore the local volume of the Milky Way via chemical and kinematical measurements from high quality astrometric and spectroscopic data recently released by the Gaia, APOGEE and GALAH programs. We chemically select 1137 stars up to 2.5~kpc of the Sun and [Fe/H]≤−1.0~dex, and find evidence of statistically significant substructures. Clustering analysis in velocity space classifies 163 objects into eight kinematical groups, whose origin is further investigated with high resolution N-body numerical simulations of single merging events.

The two retrograde groups appear associated with Gaia-Sausage-Enceladus, while the slightly prograde group could be connected to GSE or possibly Wukong. We find evidence of a new 44-member-strong prograde stream we name Icarus; to our knowledge, Icarus is the fast-rotating stream closest to the Galactic disk to date (⟨Zmax⟩≲0.5~kpc, ⟨V+VLSR⟩≃231 km s−1). Its peculiar chemical (⟨[Fe/H]⟩≃−1.45, ⟨[Mg/Fe]⟩≃−0.02) and dynamical (mean eccentricity ≃0.11) properties are consistent with the accretion of debris from a dwarf galaxy progenitor with a stellar mass of $\sim 10^9 M_\sun$ on an initial prograde low-inclination orbit, ∼10∘. The remaining prograde groups are either streams previously released by the same progenitor of Icarus (or Nyx), or remnants from different satellites accreted on initial orbits at higher inclination.

https://arxiv.org/abs/2012.10957


Sponsor: Car Rentals in Spain