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

Zhu, Ling; Pillepich, Annalisa; van de Ven, Glenn; Leaman, Ryan; Hernquist, Lars; Nelson, Dylan; Pakmor, Ruediger; Vogelsberger, Mark; Zhang, Le

doi:10.1051/0004-6361/202142496

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

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Pakmor, Ruediger
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Zhu, L., Pillepich, A., van de Ven, G., Leaman, R., Hernquist, L., Nelson, D., et al. (2022). Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass. Astronomy and Astrophysics, 660: A20. doi:10.1051/0004-6361/202142496.

Cite as: https://hdl.handle.net/21.11116/0000-000B-52FF-A

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