@article{a39b3c157d5e47a49714b8db9b9db4b2,
title = "Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass",
keywords = "Astrophysics - Astrophysics of Galaxies, galaxies, ATLAS(3D) PROJECT, data analysis, methods, SIMULATING GALAXY FORMATION, SIZE EVOLUTION, STAR-FORMATION, FORMATION HISTORY, halos, EAGLE SIMULATIONS, FORNAX3D PROJECT, LENTICULAR GALAXIES, numerical, kinematics and dynamics, ILLUSTRISTNG SIMULATIONS, ASSEMBLY HISTORIES, Methods: Numerical, Galaxies: Kinematics and dynamics, Methods: Data analysis, Galaxies: Halos",
author = "Ling Zhu and Annalisa Pillepich and {van de Ven}, Glenn and Ryan Leaman and Lars Hernquist and Dylan Nelson and Ruediger Pakmor and Mark Vogelsberger and Le Zhang",
note = "Publisher Copyright: {\textcopyright} 2022 ESO.",
year = "2022",
month = apr,
doi = "https://doi.org/10.1051/0004-6361/202142496",
language = "English",
volume = "660",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "EDP SCIENCES S A",
}