# Cold, old and metal-poor: New stellar substructures in the Milky Way's dwarf spheroidals

## TL;DR

This study identifies new and known stellar substructures in four Milky Way dwarf spheroidal galaxies, providing insights into their star formation histories and dark matter halos through advanced spatial analysis methods.

## Contribution

It introduces and applies two novel methods for detecting stellar substructures, discovering new features in Sextans and Carina dSph galaxies.

## Key findings

- Detected known substructure in Sextans
- Discovered new substructure in Sextans and Carina
- Identified multiple substructures in Leo I and Leo II

## Abstract

Dwarf spheroidal galaxies (dSph) orbiting the Milky Way are complex objects often with complicated star formation histories and internal dynamics. In this work, we search for stellar substructures in four of the classical dSph satellites of the Milky Way: Sextans, Carina, Leo I, and Leo II. We apply two methods to search for stellar substructure: the minimum spanning tree method, which helps us to find and quantify spatially connected structures, and the "brute-force" method, which is able to find elongated stellar substructures. We detected the previously known substructure in Sextans, and also found a new stellar substructure within Sextans. Furthermore, we identified a new stellar substructure close to the core radius of the Carina dwarf galaxy. We report a detection of one substructure in Leo I and two in Leo II, but we note that we are dealing with a low number of stars in the samples used. Such old stellar substructures in dSph galaxies could help us to shed light on the nature of the dark matter halos, within which such structures form, evolve, and survive.