Icarus: a Flat and Fast Prograde Stellar Stream in the Milky Way disk
Paola Re Fiorentin, Alessandro Spagna, Mario G. Lattanzi, and Michele, Cignoni

TL;DR
This paper identifies and characterizes a new prograde stellar stream named Icarus in the Milky Way, revealing its origin from a dwarf galaxy and its relation to other known structures through chemical and kinematic analysis.
Contribution
The discovery and detailed analysis of the Icarus stream, including its chemical and dynamical properties, and its association with dwarf galaxy accretion events.
Findings
Icarus is a fast-rotating, low-inclination prograde stream close to the Galactic disk.
Icarus likely originated from a dwarf galaxy with a stellar mass of about 10^9 solar masses.
Icarus's properties suggest an accretion event from a low-inclination orbit.
Abstract
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 stars up to ~kpc of the Sun and ~dex, and find evidence of statistically significant substructures. Clustering analysis in velocity space classifies 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 ($\langle…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
