Stellar Mass-to-light Ratios: Composite Bulge+Disk Models and the Baryonic Tully-Fisher Relation
arXiv:2202.02290 · doi:10.3847/1538-3881/ac5249
Abstract
We present stellar population models to calculate the mass-to-light ratio () based on galaxy's colors ranging from FUV to Spitzer IRAC1 at 3.6m. We present a new composite bulge+disk model that considers the varying contribution from bulges and disks based on their optical and near-IR colors. Using these colors, we build plausible star formation histories and chemical enrichment scenarios based on the star formation rate-stellar mass and mass-metallicity correlations for star-forming galaxies. The most accurate prescription is to use the actual colors for the bulge and disk components to constrain ; however, a reasonable bulge+disk model plus total color only introduces 5% more uncertainty. Full bulge+disk prescriptions applied to the baryonic TF relation improves the linearity of the correlation, increases the slope and reduces the total scatter by 4%.
arXiv comment22 pages, six figures, accepted by AJ
References in corpus (55)
- The epochs of early-type galaxy formation as a function of environment
- Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
- A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
- Metallicity Calibrations and the Mass-Metallicity Relation for Star-Forming Galaxies
- Galactic star formation and accretion histories from matching galaxies to dark matter haloes
- The propagation of uncertainties in stellar population synthesis modeling III: model calibration, comparison, and evaluation
- SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves
- De Re Metallica: The cosmic chemical evolution of galaxies
- Galaxy And Mass Assembly: Stellar Mass Estimates
- Resolved stellar mass maps of galaxies. I: method and implications for global mass estimates
- The Spitzer Survey of Stellar Structure in Galaxies (S^4G)
- Cosmicflows-3
- The Ursa Major Cluster of Galaxies. V ; HI Rotation Curve Shapes and the Tully-Fisher Relations
- The ACS Nearby Galaxy Survey Treasury VIII. The Global Star Formation Histories of 60 Dwarf Galaxies in the Local Volume
- Inclination- and dust-corrected galaxy parameters: Bulge-to-disc ratios and size-luminosity relations
- The DiskMass Survey. I. Overview
- The baryonic Tully-Fisher relation for different velocity definitions and implications for galaxy angular momentum
- The DiskMass Survey. VII. The distribution of luminous and dark matter in spiral galaxies
- The Formation of Disk-Bulge-Halo Systems and the Origin of the Hubble Sequence
- Chemo-spectrophotometric evolution of spiral galaxies: III. Abundance and colour gradients in discs
- On the Mass-to-Light ratio and the Initial Mass Function in disc galaxies
- The Nature of Starbursts : II. The Duration of Starbursts in Dwarf Galaxies
- New Colour-Mass to Light Relations: the role of the Asymptotic Giant Branch phase and of interstellar dust
- The Formation of a Disk Galaxy within a Growing Dark Halo
- SDSS-IV MaNGA: Global stellar population and gradients for about 2000 early-type and spiral galaxies on the mass-size plane
- Using The Baryonic Tully-Fisher Relation to Measure
- Palomar/Las Campanas Imaging Atlas of Blue Compact Dwarf Galaxies: II. Surface Photometry and the Properties of the Underlying Stellar Population
- Fundamental metallicity relation in CALIFA, SDSS-IV MaNGA and high-z galaxies
- Spitzer Local Volume Legacy (LVL) SEDs and Physical Properties
- The Star Forming Main Sequence of Dwarf Low Surface Brightness Galaxies
- The UTMOST pulsar timing programme II: Timing noise across the pulsar population
- The Origin of S0s in Clusters: evidence from the bulge and disc star formation histories
- The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
- Stellar Populations and the Star Formation Histories of LSB Galaxies: III. Stellar Population Models
- The growth of disks and bulges during hierarchical galaxy formation. I: fast evolution vs secular processes
- The Mass-to-light Ratios and the Star Formation Histories of Disk Galaxies
- AutoProf -- I. An automated non-parametric light profile pipeline for modern galaxy surveys
- Rotation curves and scaling relations of extremely massive spiral galaxies
- A duality in the origin of bulges and spheroidal galaxies
- Quantitative Morphology of Galaxies from the SDSS I: Luminosity in Bulges and Disks
- The Evolutionary History of Galactic Bulges: Photometric and Spectroscopic Studies of Distant Spheroids in the GOODS Fields
- Recovering stellar population parameters via different population models and stellar libraries
- Colors of Ellipticals from GALEX to Spitzer
- Star formation associated with neutral hydrogen in the outskirts of early-type galaxies
- SDSS-IV MaNGA: Stellar M/L gradients and the M/L-colour relation in galaxies
- Stellar Populations and the Star Formation Histories of LSB Galaxies: II. HII Regions
- Galaxy And Mass Assembly (GAMA): Galaxy colour gradients versus colour, structure and luminosity
- Fingerprints of Stellar Populations in the Near-Infrared: An Optimised Set of Spectral Indices in the JHK-Bands
- A possible solution to the [alpha/Fe]-sigma problem in early type galaxies within a hierarchical galaxy formation model
- Resolving the Disc-Halo Degeneracy II: NGC 6946
- Stellar Populations and the Star Formation Histories of LSB Galaxies: V. WFC3 Color-Magnitude Diagrams
- Dynamical measurement of the stellar surface density of face-on galaxies
- Size, shade or shape? The contribution of galaxies of different types to the star-formation history of the Universe from SDSS-IV MaNGA
- Anomalous Stellar Populations in LSB Galaxies
- The Stellar Population of Metal-Poor Galaxies at z 0.8 and the Evolution of the Mass-Metallicity Relation
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- From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
- Strong constraints on the gravitational law from DR3 wide binaries
- Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
- Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
- Radial acceleration relation of galaxies with joint kinematic and weak-lensing data
- Measuring galaxy cluster mass profiles into the low acceleration regime with galaxy kinematics
- Simulations of star forming main sequence galaxies in Milgromian gravity
- Reading the tea leaves in the - and - diagrams: dry and gaseous mergers with remnant angular momentum
- Incorporating baryon-driven contraction of dark matter halos in rotation curve fits
- Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets
- The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
- WISDOM Project -- XIII. Feeding molecular gas to the supermassive black hole in the starburst AGN-host galaxy Fairall 49
- Quashing a suspected selection bias in galaxy samples having dynamically-measured supermassive black holes
- Galactic Mass-to-Light Ratios With Superfluid Dark Matter
- Photometric vs dynamical stellar masses and their impact on scaling relations in nearby disc galaxies
- Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
- A Comparative Study of Star Forming Dwarf Galaxies using the UVIT
- Estimating the Oblateness Of Dark Matter Halos Using Neutral Hydrogen Velocity Dispersion
- Testing CCC+TL Cosmology with Galaxy Rotation Curves
- The information on halo properties contained in spectroscopic observations of late-type galaxies
- Kinematic scaling relations of disc galaxies from ionised gas at and their connection with dark matter haloes
- A positive correlation between broad HI Ly absorptions and local overdensities of galaxies
- The baryonic mass-size relation of galaxies. II. Implications for the evolutionary paths between star-forming and passive galaxies
- Star Formation Beyond the Optical Disk : The Low-Density Outskirts of NGC2090