Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass

<jats:p>Galactic dynamical structures are fossil records of the assembly histories of galaxies. By analyzing the cosmological hydrodynamical simulation TNG50, we find that a dynamical structure that we call the "hot inner stellar halo", defined by stars on dynamically hot orbits with...

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Main Authors: Zhu, Ling (Author), Pillepich, Annalisa (Author), van de Ven, Glenn (Author), Leaman, Ryan (Author), Hernquist, Lars (Author), Nelson, Dylan (Author), Pakmor, Ruediger (Author), Vogelsberger, Mark (Author), Zhang, Le (Author)
Format: Article
Language:English
Published: EDP Sciences, 2022-05-05T18:50:15Z.
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