The “Building Blocks” of Stellar Halos
The stellar halos of galaxies encode their accretion histories. In particular, the median metallicity of a halo is determined primarily by the mass of the most massive accreted object. We use hydrodynamical cosmological simulations from the apostle project to study the connection between the stellar...
Main Authors: | Kyle A. Oman, Else Starkenburg, Julio F. Navarro |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2017-08-01
|
Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/5/3/33 |
Similar Items
-
What Is Missing from the Local Stellar Halo?
by: Katherine Sharpe, et al.
Published: (2024-01-01) -
Origins of the Evil Eye: M64's Stellar Halo Reveals the Recent Accretion of an SMC-mass Satellite
by: Adam Smercina, et al.
Published: (2023-01-01) -
From Halos to Galaxies. VII. The Connections between Stellar Mass Growth History, Quenching History, and Halo Assembly History for Central Galaxies
by: Cheqiu Lyu, et al.
Published: (2023-01-01) -
Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe
by: Katya Gozman, et al.
Published: (2023-01-01) -
Resolved SPLASH Chemodynamics in Andromeda’s PHAT Stellar Halo and Disk: On the Nature of the Inner Halo along the Major Axis
by: Ivanna Escala, et al.
Published: (2023-01-01)