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MaNGA DynPop. VII. A Unified Bulge–Disk–Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-type Galaxies

Abstract:
We derive circular velocity curves (CVCs) from stellar dynamical models for ∼6000 nearby galaxies in the final data release of the Sloan Digital Sky Survey-IV MaNGA survey with integral-field spectroscopy, exploring connections between the inner gravitational potential (traced by CVC amplitude/shape) and galaxy properties. The maximum circular velocity ( Vcircmax ) and circular velocity at the half-light radius ( Vcirc(Remaj) ) both scale linearly with the stellar second velocity moment σe2≡〈V2+σ2〉 within the half-light isophote, following Vcircmax≈1.72σe (7% error) and Vcirc(Remaj)≈1.62σe (7% error). CVC shapes (rising, flat, declining) correlate strongly with structural and stellar population properties: declining curves dominate in massive, early-type, bulge-dominated galaxies with old, metal-rich stars and early quenching, while rising CVCs prevail in disk-dominated systems with younger stellar populations and ongoing star formation. Using a unified bulge–disk–halo model, we predict CVC shapes with minimal bias, identifying three governing parameters: bulge-to-total mass ratio (B/T), dark matter fraction within Re, and bulge Sérsic index. The distribution of CVC shapes across the mass–size plane reflects evolutionary pathways driven by (i) in situ star formation (spurring bulge growth) and (ii) dry mergers. This establishes CVC morphology as a diagnostic for galaxy evolution, linking dynamical signatures to structural and stellar population histories.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4365/adfb7c

Authors


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Role:
Author
ORCID:
0000-0002-2583-2669
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author
ORCID:
0000-0002-1283-8420
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Role:
Author
ORCID:
0000-0001-8317-2788
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Role:
Author
ORCID:
0000-0002-6726-9499
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Role:
Author
ORCID:
0000-0003-3899-0612


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal: Supplement Series More from this journal
Volume:
280
Issue:
2
Article number:
55
Publication date:
2025-09-23
Acceptance date:
2025-08-11
DOI:
EISSN:
1538-4365
ISSN:
0067-0049


Language:
English
Keywords:
Source identifiers:
3302452
Deposit date:
2025-09-22
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