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

Author(s)
Ling Zhu, Annalisa Pillepich, Glenn van de Ven, Ryan Leaman, Lars Hernquist, Dylan Nelson, Ruediger Pakmor, Mark Vogelsberger, Le Zhang
Organisation(s)
Department of Astrophysics
External organisation(s)
Chinese Academy of Sciences (CAS), Max-Planck-Institut für Astronomie, Harvard-Smithsonian Center for Astrophysics, Scientific Software Center, Max-Planck-Institut für Astrophysik, Massachusetts Institute of Technology
Journal
Astronomy & Astrophysics
Volume
660
No. of pages
20
ISSN
0004-6361
DOI
https://doi.org/10.1051/0004-6361/202142496
Publication date
04-2022
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Keywords
ASJC Scopus subject areas
Astronomy and Astrophysics, Space and Planetary Science
Portal url
https://ucrisportal.univie.ac.at/en/publications/a39b3c15-7d5e-47a4-9714-b8db9b9db4b2