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

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.

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Item Permalink: https://hdl.handle.net/21.11116/0000-000B-52FF-A Version Permalink: https://hdl.handle.net/21.11116/0000-000B-5300-7
Genre: Journal Article

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Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass.pdf (Any fulltext), 9MB
 
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 Creators:
Zhu, Ling, Author
Pillepich, Annalisa, Author
van de Ven, Glenn, Author
Leaman, Ryan, Author
Hernquist, Lars, Author
Nelson, Dylan, Author
Pakmor, Ruediger1, Author           
Vogelsberger, Mark, Author
Zhang, Le, Author
Affiliations:
1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882              

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Language(s): eng - English
 Dates: 2022-04-01
 Publication Status: Published online
 Pages: -
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 Table of Contents: -
 Rev. Type: -
 Identifiers: DOI: 10.1051/0004-6361/202142496
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Title: Astronomy and Astrophysics
  Other : Astron. Astrophys.
Source Genre: Journal
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Publ. Info: France : EDP Sciences S A
Pages: - Volume / Issue: 660 Sequence Number: A20 Start / End Page: - Identifier: ISSN: 1432-0746
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1