Galaxies lacking dark matter produced by close encounters in a cosmological simulation-Reference-Cited by-同舟云学术

Galaxies lacking dark matter produced by close encounters in a cosmological simulation

Published:2022-02-14 Issue:4 Volume:6 Page:496-502
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Moreno Jorge^ORCID,Danieli Shany,Bullock James S.^ORCID,Feldmann Robert^ORCID,Hopkins Philip F.,Çatmabacak Onur^ORCID,Gurvich Alexander,Lazar Alexandres^ORCID,Klein Courtney^ORCID,Hummels Cameron B.^ORCID,Hafen Zachary^ORCID,Mercado Francisco J.^ORCID,Yu Sijie^ORCID,Jiang Fangzhou^ORCID,Wheeler Coral,Wetzel Andrew^ORCID,Anglés-Alcázar Daniel^ORCID,Boylan-Kolchin Michael^ORCID,Quataert Eliot,Faucher-Giguère Claude-André^ORCID,Kereš Dušan

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01598-4.pdf

Reference56 articles.

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3. White, S. D. M. & Rees, M. J. Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering. Mon. Not. R. Astron. Soc. 183, 341–358 (1978).

4. Behroozi, P. S., Wechsler, R. H. & Conroy, C. The average star formation histories of galaxies in dark matter halos from z=0-8. Astrophys. J. 770, 57 (2013).

5. Tollerud, E. et al. From galaxy clusters to ultra-faint dwarf spheroidals: a fundamental curve connecting dispersion-supported galaxies to their dark matter halos. Astrophys. J. 726, 23 (2011).

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