Rotation Curves of Spiral Galaxies

Abstract

Rotation curves of spiral galaxies are the major tool for determining the distribution of mass in spiral galaxies. They provide fundamental information for understanding the dynamics, evolution and formation of spiral galaxies. We describe various methods to derive rotation curves, and review the results obtained. We discuss the basic characteristics of observed rotation curves in relation to various galaxy properties, such as Hubble type, structure, activity, and environment.

40 pages, 6 gif figures; Ann. Rev. Astron. Astrophys. Vol. 39, p.137, 2001

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• Vacuum stability and scalar masses in the superweak extension of the standard model
• Accretion onto a static spherically symmetric regular MOG dark compact object
• Constraints on the dark matter sound speed from galactic scales: the cases of the Modified and Extended Chaplygin Gas
• Light deflection angle through velocity profile of galaxies in $f(R)$ model
• Galaxy rotation curves with log-normal density distribution
• The diversity of spiral galaxies explained
• Testing the tensor-vector-scalar Theory with the latest cosmological observations
• Electroweakino searches at the HL-LHC in the baryon number violating MSSM
• Hawking-Like Radiation as Tunneling from a Cosmological Black Hole in Modified Gravity: Semiclassical Approximation and Beyond
• TeV-scale Majorogenesis
• The origin of double-peak emission-line galaxies: rotating discs, bars or galaxy mergers?
• Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic Systems
• The influence of dark matter halo onto the evolution of a supermassive black hole
• Radial acceleration relation and dissipative dark matter
• Nonminimal Einstein-Maxwell-Vlasov-axion model
• The ALMaQUEST survey. VIII. What causes the velocity discrepancy between CO and H$\alpha$ rotation curves in galaxies?
• Centrally Concentrated H I Distribution Enhances Star Formation in Galaxies
• Quark-antiquark confinement and nonlinear electrodynamics
• Pressure from dark matter annihilation and the rotation curve of spiral galaxies
• Rotation Curve Anomaly and Galactic Warp in M51
• On the axisymmetric thin disk model of flattened galaxies
• Radial Distributions of Surface Mass Density and Mass-to-Luminosity Ratio in Spiral Galaxies
• Pitch Angle Restrictions in Late Type Spiral Galaxies Based on Chaotic and Ordered Orbital Behavior
• Galaxy rotation curves using a non-parametric regression method: core, cusp and fuzzy scalar field dark matter models
• The flaring HI disk of the nearby spiral galaxy NGC 2683
• Flat rotation curves using scalar-tensor theories
• Search for Dark Matter Gamma-ray Emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory
• Plasma dark matter direct detection
• MeerKAT-16 HI observation of the dIrr galaxy WLM
• The line-of-sight warp of the spiral galaxy ESO 123-G23
• Dissipative dark matter halos: The steady state solution
• A thin disk in higher dimensional space-time and dark matter interpretation
• A systematic study of the inner rotation curves of galaxies observed as part of the GASS and COLD GASS surveys
• Gravity theory with a dark extra dimension
• Comparing the dark matter models, modified Newtonian dynamics and modified gravity in accounting for the galaxy rotation curves
• The `Cosmic Seagull': a highly magnified disk-like galaxy at z~2.8 behind the Bullet Cluster
• Modeling galactic halos with predominantly quintessential matter
• The SAMI Galaxy Survey: Gas Streaming and Dynamical M/L in Rotationally Supported Systems
• Going all the way in the search for WIMP dark matter at the muon collider through precision measurements
• Unveiling desert region in inert doublet model assisted by Peccei-Quinn symmetry
• Black hole mass measurement using molecular gas kinematics: what ALMA can do
• High Latitude HI in NGC 2613: Buoyant Disk-Halo Outflow
• Propagation of photons and massive vector mesons between a parity breaking medium and vacuum
• Kinematics and dynamics of the M51-type galaxy pair NGC 3893/96 (KPG 302)
• Formation of Ionization-Cone Structures in Active Galactic Nuclei: I. Stationary Model and Linear Stability Analysis
• Emergent metric and geodesic analysis in cosmological solutions of (torsion-free) Polynomial Affine Gravity
• Axions and high-energy cosmic rays: Can the relic axion density be measured?
• Internal kinematics of spiral galaxies in distant clusters III. Velocity fields from FORS2/MXU spectroscopy
• Dark Matter Fraction in z~1 Star-Forming Galaxies
• Disk galaxy scaling relations at intermediate redshifts - I. The Tully-Fisher and velocity-size relations
• Rotation curves of galactic disks for arbitrary surface density profiles: a simple and efficient recipe
• An Ap-Structure with Finslerian Flavor: I
• Distinguishing f(R) theories from general relativity by gravitational lensing effect
• Uncovering Planetary Nebulae in Early Type Galaxies using the Rutgers Fabry-Perot
• Improving sensitivity of trilinear RPV SUSY searches using machine learning at the LHC
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XI. Two dimensional H$\alpha$ kinematics of the edge-on ram pressure stripped galaxy NGC 4330
• Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
• Structure of visible and dark matter components in spiral galaxies at redshifts z = 0.5-0.9
• Stationary rotating and axially symmetric dust systems as peculiar General Relativistic objects
• Pseudo-Nambu-Goldstone Dark Matter from Non-Abelian Gauge Symmetry
• Axion-Like Dark Matter Detection Using Stern-Gerlach Interferometer
• Thermally corrected masses and freeze-in dark matter: a case study
• Astrophysical Plasma Instabilities induced by Long-Range Interacting Dark Matter
• Shan--Chen interacting vacuum cosmology
• Applying Noether's theorem to matter in the Milky Way: evidence for external perturbations and non-steady-state effects from Gaia Data Release 2
• Implications of JLA data for $k-$essence model of dark energy with given equation of state
• Nonaxisymmetric models of galaxy velocity maps
• Realising Interactions Between Dark Matter and Dark Energy Using $k$-essence Cosmology
• Is flat rotation curve a sign of cosmic expansion?
• Testing DM halos using rotation curves and lensing: A warning on the determination of the halo mass
• Dark matter inside early-type galaxies as function of mass and redshift
• 2D kinematics of the edge-on spiral galaxy ESO 379-G006
• PROBES-I: A Compendium of Deep Rotation Curves and Matched multiband Photometry
• Constraint on dark matter central density in the Eddington inspired Born-Infeld (EiBI) gravity with input from Weyl gravity
• Extremely Flat Haloes and the Shape of the Galaxy
• Interpretation of the gamma-ray excess and AMS-02 antiprotons: Velocity dependent dark matter annihilations
• An update on the two singlet Dark Matter model
• $(g-2{)}_{e,\mu }$ and strongly interacting dark matter with collider implications
• Stellar Orbital Studies in Normal Spiral Galaxies I: Restrictions to the Pitch Angle
• A simple model for explaining Galaxy Rotation Curves
• Inverse seesaw and dark matter in a gauged $\mathrm{B}-\mathrm{L}$ extension with flavour symmetry
• Effects from Dark Matter Halos on X-ray Pulsar Pulse Profiles
• OTELO survey: optimal emission-line flux determination with OSIRIS/GTC
• Electroweak Symmetry Breaking and WIMP-FIMP Dark Matter
• The imprint of arms and bars on rotation curves: in-plane and off-plane
• Dark Matter and Particle Physics
• Role of galactic bars in the formation of spiral arms: A study through orbital and escape dynamics -- I
• The interacting vacuum and tensions: a comparison of theoretical models
• Relaxation of dark matter halos: how to match observational data?
• Dark-matter-spin effects at future $e^{+}{e}^{-}$ colliders
• Constraining low scale dark hypercharge symmetry at spallation, reactor and Dark Matter direct detection experiments
• From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function
• Compact Groups analysis using weak gravitational lensing II: CFHT Stripe 82 data
• Diffusive dark matter and dark energy scenario and $k-$essence in the context of Supernova Ia observations
• Probing Brownstein-Moffat Gravity via Numerical Simulations
• How much dark matter is there inside early-type galaxies?
• Vertical stability of circular orbits in relativistic razor-thin disks
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Gravitomagnetic corrections to the lensing deflection angle for spiral galaxy models
• Kinematical asymmetry in the dwarf irregular galaxy WLM and a perturbed halo potential
• Search for ultralight dark matter with a frequency adjustable diamagnetic levitated sensor
• Jet substructure probe to unfold singlet-doublet dark matter in the presence of non-standard cosmology
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• An empirical consistent redshift bias: A possible direct reproducible observation of Zwicky's TL theory
• Theoretically motivated dark electromagnetism as the origin of relativistic MOND
• Constraints on $f(R_{ijkl}{R}^{ijkl})$ gravity: An evidence against the covariant resolution of the Pioneer anomaly
• Core-Cusp revisited and Dark Matter Phase Transition Constrained at O(0.1) eV with LSB Rotation Curve
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• Prospects of Indirect Searches for Dark Matter at INO
• GalRotpy: an educational tool to understand and parametrize the rotation curve and gravitational potential of disk-like galaxies
• Non-adiabatic evolution of dark sector in the presence of $U(1{)}_{L_{\mu }-L_{\tau }}$ gauge symmetry
• Modeling the Images of Relativistic Jets Lensed by Galaxies with Different Mass Surface Density Distributions
• Molecular Gas of the Most Massive Spiral Galaxies I: a Case Study of NGC 5908
• Comparison between two scalar field models using rotation curves of spiral galaxies
• New constraints on cosmic ray-boosted dark matter from the LUX-ZEPLIN experiment
• Spiral galaxies rotation curves in the Horava - Lifshitz gravity theory
• Explaining Xenon-1T signal with FIMP dark matter and neutrino mass in a $U(1{)}_X$ extension
• Atomic and Molecular Gas Components in Spiral Galaxies of the Virgo Cluster
• Testing the Cubic Galileon Gravity model by the Milky Way rotation curve and SPARC data
• Dwarf Galaxies without Dark Matter: constraints on Modified Gravity
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• A sensitive search for unknown spectral emission lines in the diffuse X-ray background with XMM-Newton
• Galactic phase transition at Ec=0.11 eV from rotation curves of cored LSB galaxies and nonperturbative dark matter mass
• A Molecular Gas Ring Hidden in the Sombrero Galaxy
• Complete quasinormal modes of Type-D black holes
• Resolution of the small scale structure issues with dissipative dark matter from multiple Standard Model sectors
• Highest-Resolution Rotation Curve of the Inner Milky Way proving the Galactic Shock Wave
• The Design, Implementation, and Performance of the LZ Calibration Systems
• The Gravito-Electromagnetic Approximation to the Gravimagnetic Dipole and its Velocity Rotation Curve
• Dark Sector extensions of the Littlest Seesaw in the presence of Primordial Black Holes
• New Constraints on Decaying Dark Matter from INTEGRAL/SPI
• On the galactic rotation curves problem within an axisymmetric approach
• NGC 4102: High Resolution Infrared Observations of a Nuclear Starburst Ring
• Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model
• Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
• Probing modified Newtonian dynamics with hypervelocity stars
• Reviewing the prospect of fermion triplets as dark matter and source of baryon asymmetry in non-standard cosmology
• The HI Structure of the Local Volume Dwarf Galaxy Pisces A
• Far-infrared distributions in nearby spiral galaxies NGC2841 and NGC2976 observed with AKARI/FIS
• Frequency-scanning considerations in axionlike dark matter spin-precession experiments
• Dynamics of Lyman Break Galaxies and Their Host Halos
• Dynamic domain walls in Maxwell-Dilaton background
• Domain walls in Born-Infeld-dilaton background
• Dynamical and gravitational lensing properties of a new phenomenological model of elliptical galaxies
• Stellar Orbital Studies in Normal Spiral Galaxies II: Restrictions to Structural and Dynamical parameters on Spiral Arms
• Weak lensing analysis of galaxy pairs using CS82 data
• Neutral atomic and molecular gas dynamics in the nearby spiral galaxies NGC 1512, NGC 4535, and NGC 7496
• Indirect Detection of Kaluza-Klein Dark Matter from Latticized Universal Dimensions
• Dark Matter Fraction in Disk-Like Galaxies Over the Past 10 Gyr
• Static spherically symmetric solutions of Einstein field equations with radial dark matter
• Signature of the interaction between dark sectors in the reionization process
• Capture rate of weakly interacting massive particles (WIMPs) in binary star systems
• A new constant behind the rotational velocity of galaxies
• Secluded Dark Sector and Muon $(g-2)$ in the Light of Fast Expanding Universe
• Detecting sublunar-mass primordial black holes with the Earth-Moon binary system
• Recent Observations of the Rotation of Distant Galaxies and the Implication for Dark Matter
• Results from PAMELA, ATIC and FERMI : Pulsars or Dark Matter ?
• Testing CCC+TL Cosmology with Galaxy Rotation Curves
• Reconstruction of the scalar field potential in nonmetricity gravity through Gaussian processes
• Spiral structure of the galactic disk and its influence on the rotational velocity curve
• Mass decomposition of SLACS lens galaxies in Weyl conformal gravity
• Disk Mass-to-Light ratio distribution from stellar population synthesis: Application to rotation curve decomposition of NGC 5278 (KPG 390A)
• Quantum-Enhanced Dark Matter Search Using Cat States
• Gravitational Fields of the Magnetic-type
• The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation across Space and Time in M31
• Influence of Magnetic Fields on the Gas Rotation in the Galaxy $NGC6946$
• On Filaments, Prolate Halos and Rotation Curves
• Forecasting 21-cm power spectrum sensitivity to dark Matter-baryon scattering
• Search for Axionlike Dark Matter Using Liquid-State Nuclear Magnetic Resonance
• Envelopes and vertical amplitudes of disk-crossing orbits
• Constraining A String Gauge Field by Galaxy Rotation Curves and Perihelion Precession of Planets
• Collider fingerprints of freeze-in dark matter produced during the fast expansion phase of Universe
• Modulational instabilities in neutrino--anti-neutrino interactions
• The galaxy halo formation in the absence of violent relaxation and a universal density profile of the halo center
• Global MRI with Braginskii viscosity in a galactic profile
• Probing the Scalar WIMP-Pion Coupling with the first LUX-ZEPLIN data
• Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics
• Structure and mass distribution of spiral galaxies at intermediate redshifts
• Electroweak Phase Transition, Gravitational Waves and Collider Probes in Multi-Scalar Dark Matter Scenarios
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• Mapping the distribution of luminous and dark matter in strong lensing galaxies
• Properties of cold molecular gas in four type-1 active galaxies hosting outflows
• Polynomial affine model of gravity in three-dimensions
• Rotation curves and dynamical masses of MaNGA barred galaxies
• Accretion Process as a Probe of Extra Dimensions in MOG Compact Object Spacetimes
• Photon counting for axion interferometry
• The Volumetric Star Formation Law in the Almost Edge-on Galaxy NGC 4302 Revealed by ALMA
• A simple direct empirical observation of systematic bias of the redshift as a distance indicator
• Raising galaxy rotation curves via dressing
• Can MONDian vector theories explain the cosmic speed up ?
• Shadow of quadrupole-deformed compact objects in a local dark matter shell
• Dark plasmas in the nonlinear regime: constraints from particle-in-cell simulations
• Gravitational Lensing of Euler-Heisenberg Black Hole Surrounded by Perfect Fluid Dark Matter
• Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
• Testing Cotton gravity as dark matter substitute with weak lensing
• Reply to "Comment on 'Scalar-tensor gravity coupled to a global monopole and flat rotation curves' "
• Gravity with extra dimensions and dark matter interpretation: Phenomenological example via Miyamoto-Nagai galaxy
• The Influence of Lepton Portal on the WIMP-pFIMP framework
• Exploring the evolution of structure growth in the universe with field-fluid interactions through dynamical stability analysis
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• Dynamical modelling of disc vertical structure in superthin galaxy `UGC 7321' in braneworld gravity: An MCMC study
• The Effects of Inertial Forces on the Dynamics of Disk Galaxies
• On the radial acceleration of disk galaxies
• The need for a nonlocal expansion in general relativity
• Turbulence and large-scale structures in self-gravitating superfluids
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• Chaotic orbital dynamics of pulsating stars around black holes surrounded by dark matter halos
• Virial masses of late type galaxies from the SDSS DR16
• Modified Inertia as Nonconservative Newtonian Dynamics
• Inferring halo masses with Graph Neural Networks
• When Freeze-out occurs due to a non-Boltzmann suppression: A study of degenerate dark sector
• Detecting Fluorescent Dark Matter with X-ray lasers
• Dark matter candidate induced by Horndeski theory: dark matter halo and cosmological evolution
• Observational constraints on generic models of non-minimal curvature-matter coupling
• A comprehensive dynamical and phenomenological analysis of structure growth in curvature-modulated coupled quintessence scenario
• Reconstructing Sparticle masses at the LHC using Generative Machine Learning
• The gravitational light shift and the Sachs-Wolfe effect
• Determining the surface density distribution in massive galactic disks with a central black hole
• The rotation curve and mass-distribution in highly flattened galaxies
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• Data-driven modeling of rotation curves with artificial neural networks
• Effect of dark matter halo substructures on galaxy rotation curves
• A novel approach for calculating galaxy rotation curves using spaxel cross-correlation and iterative smoothing
• Quantum-enhanced learning with a controllable bosonic variational sensor network
• RDM-stars as sources of fast radio bursts
• Timing Mass of the Local Group
• Production and constraints for a massive dark photon at electron-positron colliders
• First use of large area SiPM matrices coupled with NaI(Tl) scintillating crystal for low energy dark matter search
• Post-Newtonian properties of EMRI with Power Law Potential
• Modified scaling in $k$-essence model in interacting dark energy - dark matter scenario
• Measuring Mass of Gas in Central Galaxies using weak lensing and satellite kinematics in MOND
• Parity Breaking Medium and Squeeze Operators
• Non-minimally coupled scalar field and scaling symmetry in a cosmological background
• On the Presence of Angular-Velocity Offsets in Disk Galaxies
• Quartz fluorescence backgrounds in xenon particle detectors
• What is the amount of baryonic dark matter in galaxies?
• Probing late-time annihilations of oscillating asymmetric dark matter via rotation curves of galaxies
• A Dynamical-Photometric Phase Space for Spiral Galaxies: Probing the Local Coupling Between Light and Gravity
• Decoding the Gravitational Geometry and Stellar Photometric Profiles of Galaxy NGC 7331
• SparsePak Observations of Diffuse Ionized Gas Halo Kinematics in NGC 891
• Newtonian Gravity and Galaxy Rotation Curves: An Axisymmetric Green's Function Perspective
• Light rings, gravitational lensing, and ISCOs of exotic compact objects in Einstein-scalar-Maxwell theories
• Rotation Curve of Galaxies by the Force Induced by Mass of Moving Particles
• Spacetime of rotating black holes surrounded by massive scalar charges
• Testing subhalo abundance matching with galaxy kinematics
• SCF-FDPS: A Fast $N$-body Code for Simulating Disk-halo Systems
• A spherically symmetric gravitational solution of nearly conformally flat metric~measure~space
• Kinematic Mapping of Giant Arcs: A New Method to Locate Lensing Critical Curves
• Compact Groups in GDM Cosmological Simulations
• Scattering of quantum fields by a MOG Black Hole
• A nonlinear multiphysics model for the design validation of the ASTAROTH copper-steel cryogenic chamber
• ASTAROTH: A Novel Detector for Dark Matter Direct Detection Using Cryogenic SiPMs
• Probing Heavy Dark Matter in Red Giants
• Constraining the MOdified Newtonian Dynamics from spherically symmetrical hydrodynamic accretion
• Splitting and focusing of neutrino collective states
• Improving sensitivity of vectorlike top partner searches with jet substructure
• Can the dynamo of spiral-arm galaxies be explained by anisotropic conductivity ?
• Search for dark matter production in association with the Z${}^{\prime }$ boson at the LHC in pp collisions at $\sqrt{s}$ = 8 TeV using Monte Carlo simulations