# Evidence for a Vast Prograde Stellar Stream in the Solar Vicinity

**Authors:** Lina Necib, Bryan Ostdiek, Mariangela Lisanti, Timothy Cohen, Marat, Freytsis, Shea Garrison-Kimmel, Philip F. Hopkins, Andrew Wetzel, Robyn, Sanderson

arXiv: 1907.07190 · 2022-02-01

## TL;DR

The paper presents evidence for Nyx, a large stellar stream near the Sun, likely originating from a disrupted dwarf galaxy, revealed through Gaia data and deep learning analysis, indicating a past merger event in the Milky Way.

## Contribution

This study identifies and characterizes Nyx, a new stellar stream, using Gaia data and deep learning, providing insights into the Milky Way's merger history and stellar dynamics.

## Key findings

- Nyx is a coherent, prograde stellar stream near the Sun.
- Nyx stars have distinct kinematics, lagging the disk by ~80 km/s.
- Chemical and age data suggest Nyx originated from a dwarf galaxy.

## Abstract

Massive dwarf galaxies that merge with the Milky Way on prograde orbits can be dragged into the disk plane before being completely disrupted. Such mergers can contribute to an accreted stellar disk and a dark matter disk. We present evidence for Nyx, a vast new stellar stream in the vicinity of the Sun, that may provide the first indication that such an event occurred in the Milky Way. We identify about 500 stars that have coherent radial and prograde motion in this stream using a catalog of accreted stars built by applying deep learning methods to the second Gaia data release. Nyx is concentrated within $\pm 2$ kpc of the Galactic midplane and spans the full radial range studied (6.5-9.5 kpc). The kinematics of Nyx stars are distinct from those of both the thin and thick disk. In particular, its rotational speed lags the disk by $\sim 80$ km/s and its stars follow more eccentric orbits. A small number of Nyx stars have chemical abundances or inferred ages; from these, we deduce that Nyx stars have a peak metallicity of [Fe/H] $\sim -0.5$ and ages $\sim $10-13 Gyr. Taken together with the kinematic observations, these results strongly favor the interpretation that Nyx is the remnant of a disrupted dwarf galaxy. To further justify this interpretation, we explicitly demonstrate that metal-rich, prograde streams like Nyx can be found in the disk plane of Milky Way-like galaxies using the FIRE hydrodynamic simulations. Future spectroscopic studies will be able to validate whether Nyx stars originate from a single progenitor.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1907.07190/full.md

## Figures

13 figures with captions in the complete paper: https://tomesphere.com/paper/1907.07190/full.md

## References

54 references — full list in the complete paper: https://tomesphere.com/paper/1907.07190/full.md

---
Source: https://tomesphere.com/paper/1907.07190