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On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies

Abstract:

Observed and simulated galaxies exhibit a significant variation in their velocity dispersion profiles. We examine the inner and outer slopes of stellar velocity dispersion profiles using integral field spectroscopy data from two surveys, SAMI (for z < 0.115) and CALIFA (for z < 0.03), comparing them with results from two cosmological hydrodynamic simulations: Horizon-AGN (for z = 0.017) and NewHorizon (for z ≲ 1). The simulated galaxies closely reproduce the variety of velocity dispersion slo...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4357/ad43dc

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Role:
Author
ORCID:
0000-0001-9939-713X
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Role:
Author
ORCID:
0000-0002-4556-2619
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Role:
Author
ORCID:
0000-0002-4731-9604
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Role:
Author
ORCID:
0000-0002-5896-0034
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Role:
Author
ORCID:
0000-0003-2880-9197
Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal More from this journal
Volume:
968
Issue:
2
Article number:
96
Publication date:
2024-06-14
Acceptance date:
2024-04-24
DOI:
EISSN:
1538-4357
ISSN:
0004-637X
Language:
English
Keywords:
Source identifiers:
2042461
Deposit date:
2024-06-14

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