Shape of dark matter haloes in the Illustris simulation: effects of baryons

Chua, Kun Ting Eddie; Pillepich, Annalisa; Vogelsberger, Mark; Hernquist, Lars

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Shape of dark matter haloes in the Illustris simulation: effects of baryons

MPS-Authors

Chua, Kun Ting Eddie
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pillepich, Annalisa
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Vogelsberger, Mark
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hernquist, Lars
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2019MNRAS.484..476C
(Any fulltext)

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Chua, K. T. E., Pillepich, A., Vogelsberger, M., & Hernquist, L. (2019). Shape of dark matter haloes in the Illustris simulation: effects of baryons. Monthly Notices of the Royal Astronomical Society, 484, 476-493.

Cite as: https://hdl.handle.net/21.11116/0000-0005-D190-B

Abstract

We study the effect of baryonic processes on the shapes of dark matter (DM) haloes from Illustris, a suite of hydrodynamical (Illustris) and