NIHAO project II: halo shape, phase-space density and velocity distribution of dark matter in galaxy formation simulations-Reference-Cited by-同舟云学术

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NIHAO project II: halo shape, phase-space density and velocity distribution of dark matter in galaxy formation simulations

Published:2016-07-14 Issue:1 Volume:462 Page:663-680
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Butsky Iryna,Macciò Andrea V.,Dutton Aaron A.,Wang Liang,Obreja Aura,Stinson Greg S.,Penzo Camilla,Kang Xi,Keller Ben W.,Wadsley James

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/462/1/663/18471899/stw1688.pdf

Reference77 articles.

1. Galaxy-induced transformation of dark matter haloes

2. Fundamental differences between SPH and grid methods

3. Silicon Detector Dark Matter Results from the Final Exposure of CDMS II

4. The shape of dark matter haloes: dependence on mass, redshift, radius and formation

5. Dark Matter Results from 225 Live Days of XENON100 Data

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1. Sliding into DM: determining the local dark matter density and speed distribution using only the local circular speed of the galaxy;Journal of Cosmology and Astroparticle Physics;2024-08-01

2. Self-consistent dynamical models with a finite extent – IV. Wendland models based on compactly supported radial basis functions;Monthly Notices of the Royal Astronomical Society;2024-06-14

3. How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?;Monthly Notices of the Royal Astronomical Society;2024-01-23

4. Shaping the unseen: the influence of baryons and environment on low-mass, high-redshift dark matter haloes in the SIEGE simulations;Monthly Notices of the Royal Astronomical Society;2023-09-12

5. The oblateness of the Milky Way dark matter halo from the stellar streams of NGC 3201, M68, and Palomar 5;Monthly Notices of the Royal Astronomical Society;2023-06-27

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