Dark matter subhalo disturbance in the tidal field: Towards a new simulations accuracy-Reference-Cited by-同舟云学术

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Dark matter subhalo disturbance in the tidal field: Towards a new simulations accuracy

Published:2023-04 Issue: Volume: Page:
ISSN:2214-7853
Container-title:Materials Today: Proceedings
language:en
Short-container-title:Materials Today: Proceedings

Author:

Ahmed Ali M.,Omran Zainab H.,Taha Safa Y.,Mohammed Yahya Ayat,Jihad Mustafa A,Shehab Russul M.,Ali Al-Hilali Aqeel

Publisher

Elsevier BV

Subject

General Medicine

Reference20 articles.

1. Not so lumpy after all: modelling the depletion of dark matter subhaloes by Milky Way-like galaxies;Garrison-Kimmel;MNRAS,2017

2. 2-Banik, N., & Bovy, J. (2019). Effects of baryonic and dark matter substructure on the Pal 5 stream.Monthly Notices of the Royal Astronomical Society,484(2), 2009-2020.

3. Formation and evolution of galaxy dark matter halos and their substructure;Diemand;Astrophys. J.,2007

4. The inner structure of ΛCDM haloes–III. Universality and asymptotic slopes;Navarro;MNRAS,2004

5. Convergence and scatter of cluster density profiles;Diemand;MNRAS,2004

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