Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics
The role of baryonic physics, star formation and stellar feedback, in shaping the galaxies and their host halos is an evolving topic. The dark matter aspects are illustrated in this work by showing distribution features in a Milky Way sized halo. We focus on the halo morphology, geometry, and profil...
المؤلفون الرئيسيون: | Nuñez-Castiñeyra, A, Nezri, E, Mollitor, P, Devriendt, J, Teyssier, R |
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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
IOP Publishing
2023
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مواد مشابهة
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Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
حسب: Nuñez-Castiñeyra, A, وآخرون
منشور في: (2020) -
Analysis of dark matter profiles in the halos of spiral galaxies
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منشور في: (2023-10-01) -
The angular momentum of baryons and dark matter halos revisited
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The Baryonic Halos of Isolated Elliptical Galaxies
حسب: Ricardo Salinas, وآخرون
منشور في: (2017-08-01) -
CFHTLenS: The relation between galaxy dark matter haloes and baryons
from weak gravitational lensing
حسب: Velander, M, وآخرون
منشور في: (2013)