GaiaUnlimited: The old stellar disc of the Milky Way as traced by the Red Clump
arXiv:2410.22036 · doi:10.1051/0004-6361/202452798
Abstract
We present an exploration of the Milky Way's structural parameters using an all-sky sample of RC giants to map the stellar density from the Galactic disc beyond 3 kpc. These evolved giants are considered to be standard candles due to their low intrinsic variance in their absolute luminosities, allowing us to estimate their distances with reasonable confidence. We exploit all-sky photometry from the AllWISE mid-infrared survey and the Gaia survey, along with astrometry from Gaia Data Release 3 and recent 3D extinction maps, to develop a probabilistic scheme in order to select with high confidence RC-like stars. Our curated catalogue contains about 10 million sources, for which we estimate photometric distances based on the WISE W1 photometry. We then derive the selection function for our sample, which is the combined selection function of sources with both Gaia and AllWISE photometry. Using the distances and accounting for the full selection function of our observables, we are able to fit a two-disc, multi-parameter model to constrain the scale height (hz), scale-length (rd), flaring, and the relative mass ratios of the two disc components. We illustrate and verify our methodology using mock catalogues of RC stars. We find that the RC population is best described by a flared disc with scale length rd= kpc and scale height at the Sun of hz(at Sun)= kpc, and a shorter and thicker disc with rd= kpc, hz(at Sun)= kpc, with no flare. The thicker disc constitutes 66\% of the RC stellar mass beyond 3 kpc, while the flared disc shows evidence of being warped beyond 9 kpc from the Galactic center. The residuals between the predicted number density of RC stars from our axisymmetric model and the measured counts show possible evidence of a two-armed spiral perturbation in the disc of the Milky Way.
arXiv commentPublished in A&A, 701, A270 (2025); links to CDS data & GitHub notebooks included
References in corpus (87)
- Array Programming with NumPy
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- emcee: The MCMC Hammer
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
- Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
- Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3
- The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
- The Galaxy in Context: Structural, Kinematic and Integrated Properties
- The Milky Way Tomography with SDSS: I. Stellar Number Density Distribution
- A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS
- Kepler Mission Design, Realized Photometric Performance, and Early Science
- Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position
- The GALAH Survey: Scientific Motivation
- Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way
- Gaia Data Release 2: using Gaia parallaxes
- A distance to the Large Magellanic Cloud that is precise to one per cent
- Chemical Cartography with APOGEE: Metallicity Distribution Functions and the Chemical Structure of the Milky Way Disk
- The GALAH+ Survey: Third Data Release
- Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars
- AGAMA: Action-based galaxy modelling architecture
- LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) The survey science plan
- Estimating distances from parallaxes
- Three Dimensional Structure of the Milky Way Disk
- Vertical waves in the solar neighbourhood in Gaia DR2
- First GLIMPSE Results on the Stellar Structure of the Galaxy
- Mapping the Three-Dimensional Density of the Galactic Bulge with VVV Red Clump Stars
- The unWISE Catalog: Two Billion Infrared Sources from Five Years of WISE Imaging
- Gaia-2MASS 3D maps of Galactic interstellar dust within 3 kpc
- Galaxia: a code to generate a synthetic survey of the Milky Way
- Old stellar Galactic disc in near-plane regions according to 2MASS: scales, cut-off, flare and warp
- The Sagittarius impact as an architect of spirality and outer rings in the Milky Way
- The Milky Way's Stellar Disk
- Asteroseismology of 16000 Kepler Red Giants: Global Oscillation Parameters, Masses, and Radii
- The GALAH survey and Gaia DR2: dissecting the stellar disc's phase space by age, action, chemistry and location
- The stellar population structure of the Galactic disk
- The Spiral Structure of the Outer Milky Way in Hydrogen
- Improved GRAVITY astrometric accuracy from modeling of optical aberrations
- One Relation for All Wavelengths: The Far-Ultraviolet to Mid-Infrared Milky Way Spectroscopic R(V) Dependent Dust Extinction Relationship
- The origin of the split red clump in the Galactic bulge of the Milky Way
- Giant star seismology
- The Sixth Data Release of the Radial Velocity Experiment (RAVE) -- I: Survey Description, Spectra and Radial Velocities
- The DECam Plane Survey: Optical photometry of two billion objects in the southern Galactic plane
- Gaia Data Release 3: Mapping the asymmetric disc of the Milky Way
- Gaia Data Release 2. Cross-match with external catalogues - Algorithms and results
- Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra
- Galactic spiral structure revealed by Gaia EDR3
- An intuitive 3D map of the Galactic warp's precession traced by classical Cepheids
- StarHorse results for spectroscopic surveys + Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young-alpha rich stars
- Keeping it Cool: Much Orbit Migration, yet Little Heating, in the Galactic Disk
- Gaia Early Data Release 3: The Galactic anticentre
- Tree-ring structure of Galactic bar resonance
- Empirical photometric calibration of the Gaia Red Clump: colours, effective temperature and absolute magnitude
- The power spectrum of the Milky Way: Velocity fluctuations in the Galactic disk
- An empirical model of the Gaia DR3 selection function
- Vaex: Big Data exploration in the era of Gaia
- Red clump stars and Gaia: Calibration of the standard candle using a hierarchical probabilistic model
- Offset between stellar spiral arms and gas arms of the Milky Way
- A large and pristine sample of standard candles across the Milky Way: ~100,000 red clump stars with 3% contamination
- Trapped orbits and solar-neighbourhood kinematics
- Mapping Luminous Hot Stars in the Galaxy
- Gas and stellar spiral structures in tidally perturbed disc galaxies
- Self-consistent models of our Galaxy
- Exploring the Galactic Warp Through Asymmetries in the Kinematics of the Galactic Disk
- A Gaia early DR3 mock stellar catalog: Galactic prior and selection function
- Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. VI: An evidence for the long lived non-steady warp of non-gravitational scenarios
- Selection Functions in Astronomical Data Modeling, with the Space Density of White Dwarfs as Worked Example
- Insights from the APOKASC Determination of the Evolutionary State of Red-Giant Stars by consolidation of different methods
- Estimating the selection function of Gaia DR3 sub-samples
- Radial halo substructure in harmony with the Galactic bar
- The structural evolution of galaxies with both thin and thick discs
- Spiral-like features in the disc revealed by Gaia DR3 radial actions
- A twisted and precessing Cepheid warp in the outer Milky Way disc
- Local Spiral Structure Traced by Red Clump Stars
- The APO-K2 Catalog. II. Accurate Stellar Ages for Red Giant Branch Stars across the Milky Way
- The Great Wave: Evidence of a large-scale vertical corrugation propagating outwards in the Galactic disc
- Warp and flare of the old Galactic disc as traced by the red clump stars
- The Milky Way Bar Pattern Speed using Hercules and Gaia DR3
- The Milky Way as Seen by Classical Cepheids II: Spiral Structure
- The tangled warp of the Milky Way
- From the Inner to Outer Milky Way: A Photometric Sample of 2.6 Million Red Clump Stars
- The spiral potential of the Milky Way
- Our Galaxy's youngest disc
- Double Red Giant Branch and Red Clump features of Galactic disc stellar populations with Gaia GSPspec
- The Reduced Proper Motion selected halo: methods and description of the catalogue
- The Outer spiral arm of the Milky Way using Red Clump stars
- The GALAH Survey: Velocity fluctuations in the Milky Way using red clump giants
Cited by in corpus (2)
- Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal) II. Unveiling the formation and evolution of the kinematically selected Thick and Thin Discs
- Mapping the Milky Way with Gaia Bp/Rp spectra-IV: the broken and asymmetric density profile of the stellar disk traced by a large sample of red clumps