The Galaxy in Context: Structural, Kinematic and Integrated Properties

Abstract

Our Galaxy, the Milky Way, is a benchmark for understanding disk galaxies. It is the only galaxy whose formation history can be studied using the full distribution of stars from white dwarfs to supergiants. The oldest components provide us with unique insight into how galaxies form and evolve over billions of years. The Galaxy is a luminous (L-star) barred spiral with a central box/peanut bulge, a dominant disk, and a diffuse stellar halo. Based on global properties, it falls in the sparsely populated "green valley" region of the galaxy colour-magnitude diagram. Here we review the key integrated, structural and kinematic parameters of the Galaxy, and point to uncertainties as well as directions for future progress. Galactic studies will continue to play a fundamental role far into the future because there are measurements that can only be made in the near field and much of contemporary astrophysics depends on such observations.

69 pages, 18 figures, LaTeX. See http://www.physics.usyd.edu.au/~jbh/S/ARAA_2016.pdf for published version

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• The Milky Way Bulge: Observed properties and a comparison to external galaxies
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• A geometric distance measurement to the Galactic Center black hole with 0.3% uncertainty
• Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way
• First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
• Theoretical Challenges in Galaxy Formation
• Star Clusters Across Cosmic Time
• Gaia Data Release 2: Kinematics of globular clusters and dwarf galaxies around the Milky Way
• The GALAH+ Survey: Third Data Release
• The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
• AGAMA: Action-based galaxy modelling architecture
• Painting a portrait of the Galactic disc with its stellar clusters
• An Update on Monitoring Stellar Orbits in the Galactic Center
• Cool Outflows in Galaxies and their Implications
• The Optical to Mid-Infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS and WISE Surveys
• Mean proper motions, space orbits and velocity dispersion profiles of Galactic globular clusters derived from Gaia DR2 data
• First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment
• The Circular Velocity Curve of the Milky Way from $5$ to $25$ kpc
• Streams, substructures and the early history of the Milky Way
• Nuclear Star Clusters
• The formation and assembly history of the Milky Way revealed by its globular cluster population
• Not so lumpy after all: modeling the depletion of dark matter subhalos by Milky Way-like galaxies
• The Milky Way total mass profile as inferred from Gaia DR2
• A Unified Model for Galactic Discs: Star Formation, Turbulence Driving, and Mass Transport
• Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
• Tango for three: Sagittarius, LMC, and the Milky Way
• Proper motions and dynamics of the Milky Way globular cluster system from Gaia DR2
• The origin of accreted stellar halo populations in the Milky Way using APOGEE, $\text{Gaia}$, and the EAGLE simulations
• Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
• Markov Chain Monte Carlo Methods for Bayesian Data Analysis in Astronomy
• Gaia DR2 Proper Motions of Dwarf Galaxies within 420 kpc: Orbits, Milky Way Mass, Tidal Influences, Planar Alignments, and Group Infall
• The SAGA Survey: I. Satellite Galaxy Populations Around Eight Milky Way Analogs
• Three Hypervelocity White Dwarfs in Gaia DR2: Evidence for Dynamically Driven Double-Degenerate Double-Detonation Type Ia Supernovae
• The E-MOSAICS Project: simulating the formation and co-evolution of galaxies and their star cluster populations
• Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia EDR3 stars brighter than G=18.5
• StarHorse: A Bayesian tool for determining stellar masses, ages, distances, and extinctions for field stars
• Star-Forming Galaxies at Cosmic Noon
• A time-resolved picture of our Milky Way's early formation history
• Detection of large-scale X-ray bubbles in the Milky Way halo
• The GALAH survey and Gaia DR2: dissecting the stellar disc's phase space by age, action, chemistry and location
• The Local Group on FIRE: Dwarf galaxy populations across a suite of hydrodynamic simulations
• Evidence from APOGEE for the presence of a major building block of the halo buried in the inner Galaxy
• Mass and shape of the Milky Way's dark matter halo with globular clusters from Gaia and Hubble
• Chemodynamical history of the Galactic Bulge
• FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results
• Milky Way Satellite Census. II. Galaxy--Halo Connection Constraints Including the Impact of the Large Magellanic Cloud
• Gaia reveals a metal-rich in-situ component of the local stellar halo
• Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way
• Galactic Archaeology with asteroseismic ages: evidence for delayed gas infall in the formation of the Milky Way disc
• Improved GRAVITY astrometric accuracy from modeling of optical aberrations
• The age-metallicity structure of the Milky Way disk
• The Auriga Stellar Haloes: Connecting stellar population properties with accretion and merging history
• From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars
• Dark matter local density determination: recent observations and future prospects
• The shape of the inner Milky Way halo from observations of the Pal 5 and GD-1 stellar streams
• From the bulge to the outer disc: StarHorse stellar parameters, distances, and extinctions for stars in APOGEE DR16 and other spectroscopic surveys
• Separation of Stellar Populations by an Evolving Bar: Implications for the Bulge of the Milky Way
• VINTERGATAN I: The origins of chemically, kinematically and structurally distinct discs in a simulated Milky Way-mass galaxy
• r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos
• Reverse engineering the Milky Way
• Reconstructing the Last Major Merger of the Milky Way with the H3 Survey
• The Sixth Data Release of the Radial Velocity Experiment (RAVE) -- I: Survey Description, Spectra and Radial Velocities
• Measuring Radial Orbit Migration in the Milky Way Disk
• Farthest Neighbor: The Distant Milky Way Satellite Eridanus II
• Evidence for an Intermediate-Mass Milky Way from Gaia DR2 Halo Globular Cluster Motions
• Galactic Dark Matter Halos and Globular Cluster Populations. III: Extension to Extreme Environments
• Chemodynamics of barred galaxies in cosmological simulations: On the Milky Way's quiescent merger history and in-situ bulge
• Gaia early DR3 systemic motions of Local Group dwarf galaxies and orbital properties with a massive Large Magellanic Cloud
• Red giants observed by CoRoT and APOGEE: The evolution of the Milky Way's radial metallicity gradient
• Estimating distances from parallaxes. II. Performance of Bayesian distance estimators on a Gaia-like catalogue
• The pattern speed of the Milky Way bar from transverse velocities
• On the estimation of the Local Dark Matter Density using the rotation curve of the Milky Way
• The fraction of dark matter within galaxies from the IllustrisTNG simulations
• Ages and kinematics of chemically selected, accreted Milky Way halo stars
• Overview of the DESI Milky Way Survey
• Isochrone ages for ~3 million stars with the second Gaia data release
• Gaia Data Release 3: Mapping the asymmetric disc of the Milky Way
• Galactic Bulge Preferred Over Dark Matter for the Galactic Center Gamma-Ray Excess
• The total stellar halo mass of the Milky Way
• A White Dwarf catalogue from Gaia-DR2 and the Virtual Observatory
• The Missing Satellites of the Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-Faint Galaxies
• Globular Cluster Formation and Evolution in the Context of Cosmological Galaxy Assembly: Open Questions
• Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation
• The Extended Distribution of Baryons Around Galaxies
• Characterization and history of the Helmi streams with Gaia DR2
• An intuitive 3D map of the Galactic warp's precession traced by classical Cepheids
• Diverse Stellar Haloes in Nearby Milky Way-Mass Disc Galaxies
• Three-dimensional extinction maps: Inverting inter-calibrated extinction catalogues
• The mass of our Milky Way
• Phat ELVIS: The inevitable effect of the Milky Way's disk on its dark matter subhaloes
• A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations
• Sausage & Mash: The dual origin of the Galactic thick disc and halo from the gas-rich Gaia-Enceladus-Sausage merger
• The Hestia project: simulations of the Local Group
• The escape speed curve of the Galaxy obtained from Gaia DR2 implies a heavy Milky Way
• Revisiting the Tale of Hercules: how stars orbiting the Lagrange points visit the Sun
• Synthetic Gaia surveys from the FIRE cosmological simulations of Milky Way-mass galaxies
• The Poor Old Heart of the Milky Way
• Radial Distribution of Stellar Motions in Gaia DR2
• Early formation and recent starburst activity in the nuclear disc of the Milky Way
• Tracing the formation of the Milky Way through ultra metal-poor stars
• Resolving the Metallicity Distribution of the Stellar Halo with the H3 Survey
• The SAMI Galaxy Survey: the third and final data release
• The Milky Way bar and bulge revealed by APOGEE DR16 and Gaia EDR3
• The local high velocity tail and the Galactic escape speed
• The Proper Motion Field of the Small Magellanic Cloud: Kinematic Evidence for its Tidal Disruption
• Rotation Curves in z~1-2 Star-Forming Disks: Evidence for Cored Dark Matter Distributions
• Timing the Early Assembly of the Milky Way with the H3 Survey
• The Galactic warp revealed by Gaia DR2 kinematics
• Galactic seismology: the evolving "phase spiral" after the Sagittarius dwarf impact
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry
• Simulations of the Milky Way's central molecular zone -- I. Gas dynamics
• StarHorse results for spectroscopic surveys + Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young-alpha rich stars
• The Inside-out Growth of the Galactic Disk
• Weighing the stellar constituents of the Galactic halo with APOGEE red giant stars
• Quenching as a Contest between Galaxy Halos and their Central Black Holes
• Sample variance in the local measurements of the Hubble constant
• The origin of diverse $\alpha$-element abundances in galaxy discs
• Keeping it Cool: Much Orbit Migration, yet Little Heating, in the Galactic Disk
• Heart of Darkness: the influence of galactic dynamics on quenching star formation in galaxy spheroids
• The Gravitational Force Field of the Galaxy Measured From the Kinematics of RR Lyrae in Gaia
• Hot Atmospheres, Cold Gas, AGN Feedback and the Evolution of Early Type Galaxies: a Topical Perspective
• The ARTEMIS simulations: stellar haloes of Milky Way-mass galaxies
• Cooling flow solutions for the circumgalactic medium
• A physically motivated definition for the size of galaxies in an era of ultra-deep imaging
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• The SEDIGISM survey: first data release and overview of the Galactic structure
• The GALAH survey and Gaia DR2: Linking ridges, arches and vertical waves in the kinematics of the Milky Way
• The distribution of old stars around the Milky Way's central black hole I: Star counts
• A unified model for the maximum mass-scales of molecular clouds, stellar clusters, and high-redshift clumps
• Gaia Early Data Release 3: The Galactic anticentre
• Binary stars in the Galactic thick disc
• Fluctuations in galactic bar parameters due to bar-spiral interaction
• Gaia DR2 in 6D: Searching for the fastest stars in the Galaxy
• High-Precision Dark Halo Virial Masses from Globular Cluster Numbers: Implications for Globular Cluster Formation and Galaxy Assembly
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Observationally driven Galactic double white dwarf population for LISA
• The masses and metallicities of stellar haloes reflect galactic merger histories
• From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully-Fisher relation
• Overview of the LAMOST survey in the first decade
• Mass inflow rate into the Central Molecular Zone: observational determination and evidence of episodic accretion
• The SAMI Galaxy Survey: comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations
• The GALAH Survey: Chemical tagging and chrono-chemodynamics of accreted halo stars with GALAH+ DR3 and $Gaia$ eDR3
• Gaia EDR3 proper motions of Milky Way dwarfs I: 3D Motions and Orbits
• Spirals in galaxies
• Globular Clusters in Coma Cluster Ultra Diffuse Galaxies (UDGs): Evidence for Two Types of UDG?
• The Pristine survey X: a large population of low-metallicity stars permeates the Galactic disk
• The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• Reconstructing the Disrupted Dwarf Galaxy $Gaia$-Sausage/Enceladus Using its Stars and Globular Clusters
• Radii of Young Star Clusters in Nearby Galaxies
• Evidence of a dynamically evolving Galactic warp
• The oldest and most metal poor stars in the APOSTLE Local Group simulations
• A theoretical explanation for the Central Molecular Zone asymmetry
• The disc origin of the Milky Way bulge: Dissecting the chemo-morphological relations using N-body simulations and APOGEE
• In the Galactic disk, stellar [Fe/H] and age predict orbits and precise [X/Fe]
• How Galactic Environment affects the Dynamical State of Molecular Clouds and their Star Formation Efficiency
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• Kinematics of Highly R-Process-Enhanced Field Stars: Evidence for an Accretion Origin and Detection of Several Groups from Disrupted Satellites
• The vertical motion history of disk stars throughout the Galaxy
• COS-Burst: Observations of the Impact of Starburst-Driven Winds on the Properties of the Circum-Galactic Medium
• Updating the MACHO fraction of the Milky Way dark halo with improved mass models
• The Formation Times and Building Blocks of Milky Way-mass Galaxies in the FIRE Simulations
• Strong Evidence that the Galactic Bulge is Shining in Gamma Rays
• Searching for the 3.5 keV Line in the Deep Fields with Chandra: the 10 Ms observations
• Effects of Gas on Formation and Evolution of Stellar Bars and Nuclear Rings in Disk Galaxies
• The Accreted Nuclear Clusters of the Milky Way
• Reflex motion in the Milky Way stellar halo resulting from the Large Magellanic Cloud infall
• The mass of the Milky Way out to 100 kpc using halo stars
• How Many Components? Quantifying the Complexity of the Metallicity Distribution in the Milky Way Bulge with APOGEE
• A multi-messenger study of the Milky Way's stellar disc and bulge with LISA, Gaia and LSST
• Gaia FGK Benchmark stars: Opening the black box of stellar element abundance determination
• Blowing in the Milky Way wind: neutral hydrogen clouds tracing the Galactic nuclear outflow
• A general theory for the lifetimes of giant molecular clouds under the influence of galactic dynamics
• The physics of gas phase metallicity gradients in galaxies
• Strong constraints on thermal relic dark matter from Fermi-LAT observations of the Galactic Center
• VINTERGATAN II: the history of the Milky Way told by its mergers
• Diversity in density profiles of self-interacting dark matter satellite halos
• The Star Formation Rate of the Milky Way as seen by Herschel
• Predictions and Outcomes for the Dynamics of Rotating Galaxies
• Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
• Mapping the Milky Way with LAMOST III: Complicated spatial structure in the outer disc
• Inside Out and Upside-Down: The Roles of Gas Cooling and Dynamical Heating in Shaping the Stellar Age-Velocity Relation
• MOA-II Galactic Microlensing Constraints: The Inner Milky Way has a Low Dark Matter Fraction and a Near Maximal Disk
• Galactic Archaeology with Gaia
• Regular rotation and low turbulence in a diverse sample of z ~ 4.5 galaxies observed with ALMA
• Three Mechanisms for Bar Thickening
• The spatially-resolved star formation histories of CALIFA galaxies: Implications for galaxy formation
• APOGEE DR14/DR15 Abundances in the Inner Milky Way
• A Tale of Two Disks: Mapping the Milky Way with the Final Data Release of APOGEE
• The Need for Speed: Escape velocity and dynamical mass measurements of the Andromeda galaxy
• A relation between characteristic stellar age of galaxies and their intrinsic shape
• Galactic Archeology with the AEGIS Survey: The Evolution of Carbon and Iron in the Galactic Halo
• Massive Warm/Hot Galaxy Coronae: II. Isentropic Model
• The effect of the LMC on the Milky Way system
• Revised Geometric Estimates of the North Galactic Pole and the Sun's Height Above the Galactic Midplane
• A direct measurement of the distance to the Galactic center using the kinematics of bar stars
• MOND simulation suggests the origin of some peculiarities in the Local Group
• A Milky Way-like barred spiral galaxy at a redshift of 3
• Equilibrium models of the Milky Way mass are biased high by the LMC
• Chemodynamical Modelling of the Galactic Bulge and Bar
• Handling the Uncertainties in the Galactic Dark Matter Distribution for Particle Dark Matter Searches
• A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations
• The Pristine survey VIII: The metallicity distribution function of the Milky Way halo down to the extremely metal-poor regime
• Galaxies grow their bulges and black holes in diverse ways
• NGC5846-UDG1: A galaxy formed mostly by star formation in massive, extremely dense clumps of gas
• Revisiting long-standing puzzles of the Milky Way: the Sun and its vicinity as typical outer disk chemical evolution
• Partly burnt runaway stellar remnants from peculiar thermonuclear supernovae
• Gas Dynamics in the Galaxy: Total Mass Distribution and the Bar Pattern Speed
• The GALAH Survey: Chemodynamics of the Solar Neighbourhood
• Aurigaia: mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations
• Mapping the Galactic Metallicity Gradient with Open Clusters: The State-of-the-Art and Future Challenges
• The Dynamics of Interstellar Asteroids and Comets within the Galaxy: an Assessment of Local Candidate Source Regions for 1I/`Oumuamua and 2I/Borisov
• The Milky Way's Halo and Subhalos in Self-Interacting Dark Matter
• The Rotation Curve, Mass Distribution and Dark Matter Content of the Milky Way from Classical Cepheids
• Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys
• Gradients of chemical abundances in the Milky Way from HII regions: distances derived from Gaia EDR3 parallaxes and temperature inhomogeneities
• MINESweeper: Spectrophotometric Modeling of Stars in the Gaia Era
• The large-scale ionization cones in the Galaxy
• Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
• The Stellar Halo of the Galaxy is Tilted & Doubly Broken
• Nuclear Spirals in the inner Milky Way
• Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
• Distances, Radial Distribution and Total Number of Galactic Supernova Remnants
• A guided map to the Spiral arms in the galactic disk of the Milky Way
• The mass of our Galaxy from satellite proper motions in the Gaia era
• 2D chemical evolution model: the impact of galactic disc asymmetries on azimuthal chemical abundance variations
• The rapid onset of stellar bars in the baryon-dominated centers of disk galaxies
• Stellar mass distribution and star formation history of the Galactic disk revealed by mono-age stellar populations from LAMOST
• Barlenses and X-shape features compared: different manifestations of Boxy/Peanut bulges
• Multiple phase spirals suggest multiple origins in Gaia DR3
• A millisecond pulsar in an extremely wide binary system
• A Dynamical Mass of $70\pm 5$ Jupiter Masses for Gliese 229B, the First T Dwarf
• The geometry of the gas surrounding the Central Molecular Zone: on the origin of localised molecular clouds with extreme velocity dispersions
• Bending Waves in the Milky Way's disc from halo substructure
• Live Fast, Die Young: GMC lifetimes in the FIRE cosmological simulations of Milky Way-mass galaxies
• Under the Firelight: Stellar Tracers of the Local Dark Matter Velocity Distribution in the Milky Way
• Uncertainties in the Galactic dark matter distribution: an update
• The Magellanic Stream at 20 kpc: A New Orbital History for the Magellanic Clouds
• The Bulge Radial Velocity Assay for RR Lyrae stars (BRAVA-RR) DR2: a Bimodal Bulge?
• 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging
• Spiral arm crossings inferred from ridges in Gaia stellar velocity distributions
• The Profile of the Galactic Halo from Pan-STARRS1 3$\pi$ RR Lyrae
• Cold gas in the Milky Way's nuclear wind
• Mapping the Milky Way with LAMOST I: Method and overview
• The Bar and Spiral Arms in the Milky Way: Structure and Kinematics
• Constraining the Milky Way Mass Profile with Phase-Space Distribution of Satellite Galaxies
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• Age Dating the Galactic Bar with the Nuclear Stellar Disc
• Abundance and temperature of the outer hot circum-Galactic medium: The SRG/eROSITA view of the soft X-ray background in the eFEDS field
• Exploring the production and depletion of lithium in the Milky Way stellar disk
• The tidal remnant of an unusually metal-poor globular cluster
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• A robust estimate of the Milky Way mass from rotation curve data
• Modeling dark matter subhalos in a constrained galaxy: Global mass and boosted annihilation profiles
• Recent advances in the determination of some Galactic constants in the Milky Way
• Old, Metal-Poor Extreme Velocity Stars in the Solar Neighborhood
• Microarcsecond Astrometry: Science Highlights from Gaia
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• First direct detection constraints on Planck-scale mass dark matter with multiple-scatter signatures using the DEAP-3600 detector
• Characterizing epochs of star formation across the Milky Way disc using age-metallicity distributions of GALAH stars
• A Deep View of a Fossil Relic in the Galactic Bulge: The Globular Cluster HP1
• Astrophotonic Spectrographs
• How Many Elements Matter?
• Exploring the Galaxy's halo and very metal-weak thick disk with SkyMapper and Gaia DR2
• Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?
• Detailed Abundances for the Old Population near the Galactic Center: I. Metallicity distribution of the Nuclear Star Cluster
• The role of galactic dynamics in shaping the physical properties of giant molecular clouds in Milky Way-like galaxies
• How low does it go? Too few Galactic satellites with standard reionization quenching
• Pressure balance in the multiphase ISM of cosmologically simulated disk galaxies
• MADE: A spectroscopic Mass, Age, and Distance Estimator for red giant stars with Bayesian machine learning
• Discriminating among theories of spiral structure using Gaia DR2
• The SAMI Galaxy Survey: The internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models
• Modeling the Milky Way as a Dry Galaxy
• On the origin of the Galactic thin and thick discs, their abundance gradients and the diagnostic potential of their abundance ratios
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• Formation, vertex deviation and age of the Milky Way's bulge: input from a cosmological simulation with a late-forming bar
• The SLUGGS Survey: Measuring globular cluster ages using both photometry and spectroscopy
• Three-Dimensional Distribution of the Interstellar Dust in the Milky Way
• The tale of the tail -- disentangling the high transverse velocity stars in Gaia DR2
• Discovery of post-mass-transfer helium-burning red giants using asteroseismology
• The contribution of N-rich stars to the Galactic stellar halo using APOGEE red giants
• First Gaia dynamical model of the Milky Way disc with six phase space coordinates: a test for galaxy dynamics
• WISEA J041451.67-585456.7 and WISEA J181006.18-101000.5: The First Extreme T-type Subdwarfs?
• Diffuse Galactic antimatter from faint thermonuclear supernovae in old stellar populations
• Outflows in Star-forming Galaxies: Stacking Analyses of Resolved Winds and the Relation to Their Hosts' Properties
• The correlation between the sizes of globular cluster systems and their host dark matter haloes
• The bimodal [Mg/Fe] versus [Fe/H] bulge sequence as revealed by APOGEE DR14
• A Gaia DR 2 and VLT/FLAMES search for new satellites of the LMC
• Stellar halo substructure generated by bar resonances
• A detailed characterization of HR 8799's debris disk with ALMA in Band 7
• Discovery of disc truncations above the galaxies' mid-plane in Milky Way-like galaxies
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• Sculpting Andromeda -- made-to-measure models for M31's bar and composite bulge: dynamics, stellar and dark matter mass
• Chemical Cartography with APOGEE: Mapping Disk Populations with a Two-Process Model and Residual Abundances
• The Astrobiological Copernican Weak and Strong Limits for Extraterrestrial Intelligent Life
• The Mass of the Milky Way from the H3 Survey
• Order out of Randomness : Self-Organization Processes in Astrophysics
• Evidence for Galactic disc RR~Lyrae stars in the Solar neighbourhood
• Jeans modelling of the Milky Way's nuclear stellar disc
• Galactic Chemical Evolution of Radioactive Isotopes
• Unusual integrated metallicity profile of our Milky Way
• The phase spiral in Gaia DR3
• Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
• The Milky Way tomography with APOGEE: intrinsic density distribution and structure of mono-abundance populations
• Millimeter mapping at z~1: dust-obscured bulge building and disk growth
• Staying away from the bar: the local dynamical signature of slow and fast bars in the Milky Way
• Predicting the hypervelocity star population in Gaia
• Age-chemical abundance structure of the Galaxy I: Evidence for a late accretion event in the outer disc at z ~ 0.6
• Chemical separation of disc components using RAVE
• The Sagittarius dwarf galaxy: Where did all the gas go?
• Chemo-kinematics of the Milky Way spiral arms and bar resonances: connection to ridges and moving groups in the Solar vicinity
• An Ultra Metal-poor Star Near the Hydrogen-burning Limit
• Quantifying radial migration in the Milky Way: Inefficient over short timescales but essential to the very outer disc beyond ~15 kpc
• The structure behind the Galactic bar traced by red clump stars in the VVV survey
• Star formation history and metallicity in the Galactic inner bulge revealed by the red giant branch bump
• 591 high velocity stars in the Galactic halo selected from LAMOST DR7 and Gaia DR2
• Chemical and Kinematic Properties of the Galactic Disk from the LAMOST and Gaia Sample Stars
• The COMBS Survey -- II. Distinguishing the Metal-Poor Bulge from the Halo Interlopers
• Trojans in the Solar Neighborhood
• Gaia DR1 evidence of disrupting Perseus Arm
• The GALAH survey: properties of the Galactic disk(s) in the solar neighbourhood
• Milky Way total Mass derived by Rotation Curve and Globular Cluster kinematics from Gaia EDR3
• Great Balls of FIRE I: The formation of star clusters across cosmic time in a Milky Way-mass galaxy
• Galactic Rotation from Cepheids with Gaia DR2 and Effects of Non-Axisymmetry
• Joint constraints on the Galactic dark matter halo and Galactic Centre from hypervelocity stars
• Dynamically Driven Inflow onto the Galactic Center and its Effect upon Molecular Clouds
• Identifying kinematic structures in simulated galaxies using unsupervised machine learning
• Aluminum Enhanced Metal-Poor Stars buried in the Inner Galaxy
• The bursty star formation history of the Fornax dwarf spheroidal galaxy revealed with the HST
• 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
• Buoyant crystals halt the cooling of white dwarf stars
• A Tilted Dark Halo Origin of the Galactic Disk Warp and Flare
• Trimodal structure of Hercules stream explained by originating from bar resonances
• The VMC Survey -- XLVIII. Classical Cepheids unveil the 3D geometry of the LMC
• Testing kinematic distances under a realistic Galactic potential
• Streams on FIRE: Populations of Detectable Stellar Streams in the Milky Way and FIRE
• Milky Way Mass with K Giants and BHB Stars Using LAMOST, SDSS/SEGUE, and Gaia: 3D Spherical Jeans Equation and Tracer Mass Estimator
• Exploring the origin of thick disks using the NewHorizon and Galactica simulations
• A revisit of PSR J1909$-$3744 with 15-year high-precision timing
• Figuring Out Gas & Galaxies In Enzo (FOGGIE). IV. The Stochasticity of Ram Pressure Stripping in Galactic Halos
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• Connecting the Milky Way potential profile to the orbital timescales and spatial structure of the Sagittarius Stream
• The velocity anisotropy of the Milky Way satellite system
• Abundances in the Milky Way across five nucleosynthetic channels from 4 million LAMOST stars
• Gaia Data Release 3: A Golden Sample of Astrophysical Parameters
• The geometry of the magnetic field in the Central Molecular Zone measured by PILOT
• A Parametric Galactic Model toward the Galactic Bulge Based on Gaia and Microlensing Data
• Core-Collapse Supernovae in Binaries as the Origin of Galactic Hyper-Runaway Stars
• The Gaia-ESO Survey: the selection function of the Milky Way field stars
• Gaia EDR3 in 6D: Searching for unbound stars in the Galaxy
• Mapping the Galactic disk with the LAMOST and $Gaia$ Red clump sample: V: On the origin of the "young" [$\alpha$/Fe]-enhanced stars
• Exploring the pertubed Milky Way disk and the substructures of the outer disk
• The stellar velocity distribution function in the Milky Way galaxy
• Chronology of our Galaxy from Gaia Colour-Magnitude Diagram-fitting (ChronoGal). I. The formation and evolution of the thin disk from the Gaia Catalogue of Nearby Stars
• Tracing the Milky Way warp and spiral arms with classical Cepheids
• Globular cluster systems and galaxy formation
• Ruprecht 147: a paradigm of dissolving star cluster
• Relations among structural parameters in barred galaxies with a direct measurement of bar pattern speed
• Gravitational Wave Radiation of Double Degenerates with Extremely low-mass WD companions
• The Three-Phase Evolution of the Milky Way
• Bar effect on gas-phase abundance gradients. I. Data sample and chemical abundances
• Abundances of disk and Bulge giants from high-resolution optical spectra III. Sc, V, Cr, Mn, Co, Ni
• The aftermath of the Great Collision between our Galaxy and the Large Magellanic Cloud
• Strong chemical tagging with APOGEE: 21 candidate star clusters that have dissolved across the Milky Way disc
• Mapping the Milky Way with LAMOST II: the stellar halo
• Population syntheses of millisecond pulsars from the Galactic Disk and Bulge
• RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic Scales
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• The kinematics of the outer halo of M87 as mapped by planetary nebulae
• Stars that Move Together Were Born Together
• Galaxy and Mass Assembly (GAMA): Variation in Galaxy Structure Across the Green Valley
• The GALAH Survey: Chemical Clocks
• Action-based distribution function modelling for constraining the shape of the Galactic dark matter halo
• The CGM${}^2$ Survey: Circumgalactic O VI from dwarf to massive star-forming galaxies
• The history of the dark and luminous side of Milky Way-like progenitors
• Gravitational Waves from Double White Dwarfs as probes of the Milky Way
• A variational encoder-decoder approach to precise spectroscopic age estimation for large Galactic surveys
• A Statistical Analysis of Galactic Radio Supernova Remnants
• The GALAH Survey: Stellar streams and how stellar velocity distributions vary with Galactic longitude, hemisphere and metallicity
• A high pitch angle structure in the Sagittarius Arm
• Proper Motion of the Leo II Dwarf Galaxy Based On Hubble Space Telescope Imaging
• Galactic Bar Resonances Inferred from Kinematically Hot Stars in Gaia EDR3
• Chemo-kinematics of the Milky Way from the SDSS-III MARVELS Survey
• Kinematics in the Galactic Bulge with APOGEE: II. High-Order Kinematical Moments and Comparison to Extragalactic Bar Diagnostics
• Mass models of the Milky Way and estimation of its mass from the GAIA DR3 data-set
• The Effective J-Factor of the Galactic Center for Velocity-Dependent Dark Matter Annihilation
• The Magellanic System: the puzzle of the leading gas stream
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• New Limits on Charged Dark Matter from Large-Scale Coherent Magnetic Fields
• New nearby hypervelocity stars and their spatial distribution from Gaia DR2
• High-energy gamma-ray and neutrino production in star-forming galaxies across cosmic time: Difficulties in explaining the IceCube data
• Most "young" $\alpha$-rich stars have high masses but are actually old
• From giant clumps to clouds -- II. The emergence of thick disc kinematics from the conditions of star formation in high redshift gas rich galaxies
• Kinematic properties of white dwarfs. Galactic orbital parameters and age-velocity dispersion relation
• Global Properties of M31's Stellar Halo from the SPLASH Survey: III. Measuring the Stellar Velocity Dispersion Profile
• The impact of early massive mergers on the chemical evolution of Milky Way-like galaxies: insights from NIHAO-UHD simulations
• On the stability of tidal streams in action space
• Statistical detection of a tidal stream associated with the globular cluster M68 using Gaia data
• Yule-Simpson's paradox in Galactic Archaeology
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• Estimating stellar ages and metallicities from parallaxes and broadband photometry - successes and shortcomings
• Bootes III is a disrupting dwarf galaxy associated with the Styx stellar stream
• A seismic scaling relation for stellar age
• Identifying Interstellar Objects Trapped in the Solar System through Their Orbital Parameters
• Probing the Milky Way's Dark Matter Halo for the 3.5 keV Line
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• A New Estimate of the Best Value for the Solar Galactocentric Distance
• Local RR Lyrae Stars: native and alien
• Metal-poor Stars Observed with the Automated Planet Finder Telescope. II. Chemodynamical Analysis of Six Low-Metallicity Stars in the Halo System of the Milky Way
• The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics
• Using classical Cepheids to study the far side of the Milky Way disk: I. Spectroscopic classification and the metallicity gradient
• First constraints on Fuzzy Dark Matter from the dynamics of stellar streams in the Milky Way
• Constraining the Galactic structure parameters with the XSTPS-GAC and SDSS photometric surveys
• Figuring Out Gas & Galaxies in Enzo (FOGGIE). III. The Mocky Way: Investigating Biases in Observing the Milky Way's Circumgalactic Medium
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• The K2 Galactic Caps Project -- Going Beyond the \textit{Kepler} Field and Ageing the Galactic Disc
• An ever-present $Gaia$ snail shell triggered by a dark matter wake
• Solo dwarfs III: Exploring the orbital origins of isolated Local Group galaxies with Gaia Data Release 2
• Dynamical model of the Milky Way using APOGEE and Gaia data
• Milky Way Analogues in MaNGA: Multi-Parameter Homogeneity and Comparison to the Milky Way
• What the Milky Way bulge reveals about the initial metallicity gradients in the disc
• Constraining the pitch angle of the Galactic spiral arms in the Milky Way
• Quantifying the (X/peanut)-shaped Structure of the Milky Way - New Constraints on the Bar Geometry
• Neutrino clustering in the Milky Way and beyond
• The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas
• Radial halo substructure in harmony with the Galactic bar
• JWST-TST Proper Motions: I. High-Precision NIRISS Calibration and Large Magellanic Cloud Kinematics
• Continuous gravitational waves from Galactic neutron stars: demography, detectability and prospects
• Regulation of Star Formation by a Hot Circumgalactic Medium
• The Pristine Inner Galaxy Survey (PIGS) V: a chemo-dynamical investigation of the early assembly of the Milky Way with the most metal-poor stars in the bulge
• The Fornax3D project: discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427
• Chemical Evolution with Radial Mixing Redux: Extending beyond the Solar Neighborhood
• Comparing the Galactic Bulge and Galactic Disk Millisecond Pulsars
• Three-dimensional structure of the milky way dust: modeling of LAMOST data
• GaiaNIR: Combining optical and Near-Infra-Red (NIR) capabilities with Time-Delay-Integration (TDI) sensors for a future Gaia-like mission
• Vertical Phase Mixing across the Galactic Disk
• Are the Milky Way and Andromeda unusual? A comparison with Milky Way and Andromeda Analogs
• X-ray and SZ constraints on the properties of hot CGM
• Sensitivity projections for a dual-phase argon TPC optimized for light dark matter searches through the ionization channel
• Exploring the spectral \textit{information content} in the LAMOST medium-resolution survey (MRS)
• A population of galaxy-scale jets discovered using LOFAR
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• The central spheroids of Milky Way mass-sized galaxies
• Predictably Missing Satellites: Subhalo Abundance in Milky Way-like Halos
• Using Torque to Understand Barred Galaxy Models
• The Galactic Center as a laboratory for theories of gravity and dark matter
• RR Lyrae-based Distances for 39 Nearby Dwarf Galaxies Calibrated to Gaia eDR3
• Bar pattern speeds in CALIFA galaxies III. Solving the puzzle of ultrafast bars
• An artificial neural network to discover Hypervelocity stars: Candidates in Gaia DR1/TGAS
• Characteristics of the two sequences seen in the high-velocity Hertzsprung-Russell diagram in Gaia DR2
• Tracing the anemic stellar halo of M101
• The Magellanic Edges Survey I. Description and First Results
• Orbits of selected globular clusters in the Galactic bulge
• The accreted stellar halo as a window on halo assembly in L* galaxies
• Chemical Cartography. II. The Assembly History of the Galactic Stellar Halo Traced by Carbon-Enhanced Metal-Poor Stars
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• Origin of highly $r$-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
• Galactic seismology: joint evolution of impact-triggered stellar and gaseous disc corrugations
• Quantifying the effects of spatial resolution and noise on galaxy metallicity gradients
• The fastest stars in the Galaxy
• Kinematics of RR Lyrae stars in the Galactic bulge with OGLE-IV and Gaia DR2
• Effects of galaxy--satellite interactions on bar formation
• Migration in the shearing sheet and estimates for young open cluster migration
• The structural evolution of galaxies with both thin and thick discs
• The survey of planetary nebulae in Andromeda (M 31) V. Chemical enrichment of the thin and thicker discs of Andromeda. Oxygen to argon abundance ratios for planetary nebulae and H II regions
• Chemical and kinematic analysis of CN-strong Metal-poor Field Stars in LAMOST DR3
• Testing Dark Matter and Modifications to Gravity using Local Milky Way Observables
• Orbital Torus Imaging: Using Element Abundances to Map Orbits and Mass in the Milky Way
• Molecular gas distribution perpendicular to the Galactic plane
• A Dynamical Model for Clustered Star Formation in the Galactic Disk
• Using Commensurabilities and Orbit Structure to Understand Barred Galaxy Evolution
• VVVX-Gaia Discovery of a Low Luminosity Globular Cluster in the Milky Way Disk
• Stellar Accelerations and the Galactic Gravitational Field
• SRG/eROSITA X-ray shadowing study of giant molecular clouds
• Structure and kinematics of Type II Cepheids in the Galactic bulge based on near-infrared VVV data
• Detailed abundance analysis of a metal-poor giant in the Galactic Center
• A KMOS survey of the nuclear disk of the Milky Way I: Survey design and metallicities
• Milky Way thin and thick disk kinematics with GAIA EDR3 and RAVE DR5
• The Sheet of Giants: Unusual Properties of the Milky Way's Immediate Neighbourhood
• How cosmological merger histories shape the diversity of stellar haloes
• A model for the minimum mass of bound stellar clusters and its dependence on the galactic environment
• NuSTAR + XMM-Newton monitoring of the neutron star transient AX J1745.6-2901
• First metallicity determination from Near-Infrared spectra for five obscured Cepheids discovered in the inner Disk
• Establishing the Galactic Centre Distance Using VVV Bulge RR Lyrae Variables
• SRG/eROSITA discovery of a large circular SNR candidate G116.6-26.1: SN Ia explosion probing the gas of the Milky Way halo?
• Migration and kinematics in growing disc galaxies with thin and thick discs
• Autonomous Gaussian decomposition of the Galactic Ring Survey. I. Global statistics and properties of the 13CO emission data
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• Gaia's Detectability of Black Hole-Main Sequence Star Binaries Formed in Open Clusters
• Spiral-like features in the disc revealed by Gaia DR3 radial actions
• Prompt cusps and the dark matter annihilation signal
• Orbital dynamics and histories of satellite galaxies around Milky Way-mass galaxies in the FIRE simulations
• The formation and survival of the Milky Way's oldest stellar disk
• Metallicity distributions of halo stars: do they trace the Galactic accretion history?
• An extremely low mid-infrared extinction law toward the Galactic Center and 4% distance precision to 55 classical Cepheids
• An [$\alpha$/Fe]-enhanced thick disk in a Milky Way Analogue
• Substructure at High Speed II: The Local Escape Velocity and Milky Way Mass with Gaia DR2
• The kinematic signature of the Galactic warp in Gaia DR1 - I. The Hipparcos subsample
• The Life Cycle of the Central Molecular Zone. II: Distribution of atomic and molecular gas tracers
• Maximum Entropy Estimation of the Galactic Bulge Morphology via the VVV Red Clump
• Mira variables in the Milky Way's nuclear stellar disc: discovery and classification
• Towards sub-kpc scale kinematics of molecular and ionized gas of star-forming galaxies at $z\sim 1$
• Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
• The survey of planetary nebulae in Andromeda (M31). IV. Radial oxygen and argon abundance gradients of the thin and thicker disc
• Models of rotating coronae
• Clustering of Local Group distances: publication bias or correlated measurements? V. Galactic rotation constants
• A census of new globular clusters in the Galactic bulge
• Origin of Spin-Orbit Misalignments: The Microblazar V4641 Sgr
• The Imprint of Spiral Arms on the Galactic Rotation Curve
• Phase-space Properties and Chemistry of the Sagittarius Stellar Stream Down to the Extremely Metal-poor ($[Fe/H]\lesssim -3$) Regime
• The Unmixed Debris of Gaia-Sausage/Enceladus in the Form of a Pair of Halo Stellar Overdensities
• The Milky Way's rotation curve with superfluid dark matter
• 7.1 keV sterile neutrino dark matter constraints from a deep Chandra X-ray observation of the Galactic bulge Limiting Window
• Cataloging Accreted Stars within Gaia DR2 using Deep Learning
• Formation imprints in the kinematics of the Milky Way globular cluster system
• Weighing the Galactic disk using phase-space spirals III. Probing distant regions of the disk using the Gaia EDR3 proper motion sample
• Determination of Dark Matter Halo Mass from Dynamics of Satellite Galaxies
• The Milky Way's bar structural properties from gravitational waves
• The velocity ellipsoid in the Galactic disc using Gaia DR1
• The Flare and Warp of the Young Stellar Disk traced with LAMOST DR5 OB-type stars
• A VLBI distance and transverse velocity for PSR B1913+16
• Milky Way globular clusters on cosmological timescales. I. Evolution of the orbital parameters in time-varying potentials
• Composite Bulges -- II. Classical Bulges and Nuclear Discs in Barred Galaxies: The Contrasting Cases of NGC 4608 and NGC 4643
• Empirical Constraints on the Nucleosynthesis of Nitrogen
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• Sumo Puff: Tidal Debris or Disturbed Ultra-Diffuse Galaxy?
• The most metal-poor Galactic globular cluster: the first spectroscopic observations of ESO280-SC06
• A Hunt for Magnetic Signatures of Hidden-Photon and Axion Dark Matter in the Wilderness
• The Missing Satellite Problem Outside of the Local Group: I -- Pilot Observation
• Using classical Cepheids to study the far side of the Milky Way disk. II. The spiral structure in the first and fourth Galactic quadrants
• Using the Multi-Object Adaptive Optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre
• A2A: 21,000 bulge stars from the ARGOS survey with stellar parameters on the APOGEE scale
• A first estimate of the Milky Way dark matter halo spin
• The energy distribution of the first supernovae
• The oblateness of the Milky Way dark matter halo from the stellar streams of NGC 3201, M68, and Palomar 5
• Combined dynamical effects of the bar and spiral arms in a Galaxy model. Application to the solar neighbourhood
• Helium abundances and its radial gradient from the spectra of HII regions and ring nebulae of the Milky Way
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• Weighing the Galactic disk in sub-regions of the solar neighbourhood using Gaia DR2
• GASKAP Pilot Survey Science II: ASKAP Zoom Observations of Galactic 21-cm Absorption
• Was the Milky Way a chain galaxy? Using the IGIMF theory to constrain the thin-disk star formation history and mass
• Hidden in the Haystack: Low-luminosity globular clusters towards the Milky Way bulge
• From ridges to manifolds: 3D characterization of the moving groups in the Milky Way disc
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Declining rotation curves at $z=2$ in $\Lambda$CDM galaxy formation simulations
• Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model
• The high velocity stars in the Local Stellar Halo from Gaia and LAMOST
• Planet formation throughout the Milky Way: Planet populations in the context of Galactic chemical evolution
• The e-TidalGCs Project: Modeling the extra-tidal features generated by Galactic globular clusters
• From the Outside Looking in: What can Milky Way Analogues Tell us About the Star Formation Rate of Our Own Galaxy?
• Young stars as tracers of a barred-spiral Milky Way
• Self-consistent dust and non-LTE line radiative transfer with SKIRT
• Milky Way archaeology using RR Lyrae and type II Cepheids II. High velocity RR Lyrae stars, and mass of the Milky Way
• Impact of distance determinations on Galactic structure. I. Young and intermediate-age tracers
• Gamma-ray emission from the Sagittarius Dwarf Spheroidal galaxy due to millisecond pulsars
• Beyond Ultra-diffuse Galaxies. I. Mass--Size Outliers among the Satellites of Milky Way Analogs
• Constraining a companion of the galactic center black hole, Sgr A*
• An excessively massive thick disc of the enormous edge-on lenticular galaxy NGC7572
• Formation of supermassive black holes in galactic nuclei II: retention and growth of seed intermediate-mass black holes
• Stellar Overdensity in the Local Arm in Gaia DR2
• The far side of the Galactic bar/bulge revealed through semi-regular variables
• The Ages and Metallicities of the Globular Clusters in the Sparkler
• Constraining the Milky Way assembly history with Galactic Archaeology. Ludwig Biermann Award Lecture 2015
• The nature of the Milky Way's stellar halo revealed by the three integrals of motion
• Modelling the Milky Way. I -- Method and first results fitting the thick disk and halo with DES-Y3 data
• Spitzer Infrared Spectrograph Observations of the Galactic Center: Quantifying the Extreme Ultraviolet/so ft X-ray fluxes
• Detectablity of Black Hole Binaries with Gaia: Dependence on Binary Evolution Models
• Which Milky Way masses are consistent with the slightly declining 5-25 kpc rotation curve?
• The Most Metal-poor Stars in the Inner Bulge
• The Coupling of Galactic Dark Matter Halos with Stellar Bars
• Galactic googly: the rotation-metallicity bias in the inner stellar halo of the Milky Way
• The Pristine survey -- XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations
• Impact of galactic distributions in celestial capture of dark matter
• The GECKOS Survey: Identifying kinematic sub-structures in edge-on galaxies
• Influence of a mass transfer stability criterion on double white dwarf populations
• The course of the Orphan Stream in the Northern Galactic Hemisphere traced with Gaia DR2
• Age dissection of the vertical breathing motions in Gaia DR2: evidence for spiral driving
• The substructures in the local stellar halo from Gaia and LAMOST
• Spin-dependent sub-GeV Inelastic Dark Matter-electron scattering and Migdal effect: (I). Velocity Independent Operator
• Tidally stripped halo stars from the Large Magellanic Cloud in the Galactic North
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• Observational Constraints of Radial Migration in the Galactic Disc Driven by the Slowing Bar
• SiO Masers in the Galactic Bulge and Disk: Kinematics from the BAaDE Survey
• Gaia DR3 features of the phase spiral and its possible relation to internal perturbations
• Halo uncertainties in electron recoil events at direct detection experiments
• The Second Nucleus of NGC 7727: Direct Evidence for the Formation and Evolution of an Ultracompact Dwarf Galaxy
• The GALAH Survey: Accreted stars also inhabit the Spite Plateau
• A Bayesian estimation of the Milky Way's circular velocity curve using Gaia DR3
• Discovery of A candidate Hypervelocity star originated from the Sagittarius Dwarf Spheroidal galaxy
• First Constraints on WIMP-Nucleon Effective Field Theory Couplings in an Extended Energy Region From LUX-ZEPLIN
• Voyage through the Hidden Physics of the Cosmic Web
• The black hole retention fraction in star clusters
• The metal-rich halo component extended in z: a characterization with Gaia DR2 and APOGEE
• On the Flaring of Thick Disc of Galaxies: Insights from Simulations
• Effects of the Central Mass Concentration on Bar Formation in Disk Galaxies
• Exploring the Dust Content of Galactic Halos with Herschel III. NGC 891
• The cosmic ray ionisation and $\gamma$-ray budgets of star-forming galaxies
• Warp and flare of the old Galactic disc as traced by the red clump stars
• On the origins of extreme velocity stars as revealed by large-scale Galactic surveys
• Structural Analogs of the Milky Way Galaxy: Stellar Populations in the Boxy Bulges of NGC 4565 and NGC 5746
• The structure of the Milky Way based on unWISE 3.4$\mu$m integrated photometry
• Evidence of a Flat Outer Rotation Curve in a Starbursting Disk Galaxy at $z=1.6$
• Universal properties of the high- and low-α disk: small intrinsic abundance scatter and migrating stars
• The non-explosive stellar merging origin of the ultra-massive carbon-rich white dwarfs
• The Great Wave: Evidence of a large-scale vertical corrugation propagating outwards in the Galactic disc
• The imprint of clump formation at high redshift. II. The chemistry of the bulge
• SMHASH: Anatomy of the Orphan Stream using RR Lyrae stars
• Dark Matter Microhalos in the Solar Neighborhood: Pulsar Timing Signatures of Early Matter Domination
• MSA-3D: Metallicity Gradients in Galaxies at $z\sim 1$ with JWST/NIRSpec Slit-stepping Spectroscopy
• Realistic HI scale heights of Milky Way-mass galaxies in the FIREbox cosmological volume
• Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski~2)
• The Globular Cluster Origin of the Milky Way Outer Bulge: Evidence from Sodium Bimodality
• Extending the Chemical Reach of the H3 Survey: Detailed Abundances of the Dwarf-galaxy Stellar Stream Wukong/LMS-1
• Gravitational lensing of massive particles by a black-bounce-Schwarzschild black hole
• Distribution and kinematics of 26Al in the Galactic disc
• The effect of Large Magellanic Cloud on the satellite galaxy population in Milky Way analogous Galaxies
• Detailed study of the Milky Way globular cluster Laevens 3
• Linking the formation and fate of exo-Kuiper belts within solar system analogues
• Kinematic footprint of the Milky Way spiral arms in Gaia EDR3
• The dark side of FIRE: predicting the population of dark matter subhaloes around Milky Way-mass galaxies
• Study of the excess Fe XXV line emission in the central degrees of the Galactic centre using XMM-Newton data
• Chemical Evolution of Ytterbium in the Galactic Disk
• The Proper Motion of Pyxis: the first use of Adaptive Optics in tandem with HST on a faint halo object
• Testing MOdified Gravity (MOG) theory and dark matter model in Milky Way using the local observables
• Modelling the stellar halo with RR-Lyrae stars
• The QuaStar Survey: Detecting Hidden Low-Velocity Gas in the Milky Way's Circumgalactic Medium
• Deep Potential: Recovering the gravitational potential from a snapshot of phase space
• Constraining the primordial curvature perturbation using dark matter substructure
• A kinematic calibration of the O-rich Mira variable period-age relation from Gaia
• Informing dark matter direct detection limits with the ARTEMIS simulations
• The M31/M33 tidal interaction: A hydrodynamic simulation of the extended gas distribution
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• The Galactic neutron star population I - an extragalactic view of the Milky Way and the implications for fast radio bursts
• Can ultralight dark matter explain the age-velocity dispersion relation of the Milky Way disc: A revised and improved treatment
• Comparing hypervelocity star populations from the Large Magellanic Cloud and the Milky Way
• Probing the early Milky Way with GHOST spectra of an extremely metal-poor star in the Galactic disk
• The origin of high velocity stars from Gaia and LAMOST
• The Smith Cloud: surviving a high speed transit of the Galactic disc
• The impact of metallicity on nova populations
• The Orbit and Origin of the Ultra-faint Dwarf Galaxy Segue 1
• Detecting the Figure Rotation of Dark Matter Halos with Tidal Streams
• Predicting the Yield of Small Transiting Exoplanets around Mid-M and Ultra-Cool Dwarfs in the Nancy Grace Roman Space Telescope Galactic Bulge Time Domain Survey
• The Age-Metallicity-Specific Orbital Energy Relation for the Milky Way's Globular Cluster System Confirms the Importance of Accretion for Its Formation
• Robust inference of the Galactic centre gamma-ray excess spatial properties
• Spatial Distribution of Globular Clusters in the Galaxy
• Sizing from the Smallest Scales: The Mass of the Milky Way
• Halo intruders in the Galactic bulge revealed by HST and Gaia: the globular clusters Terzan 10 and Djorgovski 1
• Dwarfs in the Milky Way halo outer rim: first in-fall or backsplash satellites?
• The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs
• Proper motions of OB stars in the far Carina Arm
• The VVV survey: Long-period variable stars I. Photometric catalog of ten VVV/OGLE tiles
• PANORAMIC: Discovery of an Ultra-Massive Grand-Design Spiral Galaxy at $z\sim 5.2$
• Barlenses in the CALIFA survey: combining the photometric and stellar population analysis
• GalMod: a Galactic synthesis population model
• Chandra large-scale mapping of the Galactic center: Probing high-energy structures around the central molecular zone
• A purely acceleration-based measurement of the fundamental Galactic parameters
• Dynamics of Stellar Disk Tilting from Satellite Mergers
• The Mira-based distance to the Galactic centre
• A slightly oblate dark matter halo revealed by a retrograde precessing Galactic disk warp
• Cardinal kinematics: I. Rotation fields of the APOGEE Survey
• Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-Time Distribution
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• The orbital evolution of UFDs and GCs in an evolving Galactic potential
• The [Y/Mg] chemical clock in the Galactic Disk: The influence of metallicity and Galactic population in the solar neighbourhood
• A Deep, High-Angular Resolution 3D Dust Map of the Southern Galactic Plane
• Asymmetric eROSITA bubbles as the evidence of a circumgalactic medium wind
• The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
• Hot atmospheres of galaxies, groups, and clusters of galaxies
• Properties of the Magellanic Corona
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• The HR 1614 moving group is not a dissolving cluster
• The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6
• On the metal-poor edge of the Milky Way "thin disc"
• The effect of stellar encounters on the dark matter annihilation signal from prompt cusps
• The Gaia-ESO Survey: Old super-metal-rich visitors from the inner Galaxy
• Discovery of s-process enhanced stars in the LAMOST survey
• Bulge formation through disc instability -- I
• All-Sky Kinematics of the Distant Halo: The Reflex Response to the LMC
• Inverse Compton emission from millisecond pulsars in the Galactic bulge
• Remarkable migration of the solar system from the innermost Galactic disk; a wander, a wobble, and a climate catastrophe on the Earth
• The Implications of Local Fluctuations in the Galactic Midplane for Dynamical Analysis in the Gaia Era
• The retrograde orbit of the globular cluster FSR1758 revealed with Gaia DR2
• The vertical force in the Solar Neighbourhood using red clump stars in TGASxRAVE - Constraints on the local dark matter density
• The hELENa project - II. Abundance distribution trends of early-type galaxies: from dwarfs to giants
• The formation of subdwarf A-type stars
• Measuring the Orbits of the Arches and Quintuplet Clusters using HST and Gaia: Exploring Scenarios for Star Formation Near the Galactic Center
• On the Oosterhoff dichotomy in the Galactic bulge: II. kinematical distribution
• Modeling of Spiral Structure in a Multi-Component Milky~Way-Like Galaxy
• Action-based Dynamical Modeling for the Milky Way Disk: The Influence of Spiral Arms
• Precise Ages of Field Stars From White Dwarf Companions in Gaia DR2
• Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
• ALMA uncovers highly filamentary structure towards the Sgr E region
• Ultracool dwarfs identified using spectra in LAMOST DR7
• Manifold spirals, disc-halo interactions and the secular evolution in N-body models of barred galaxies
• The outermost edges of the Milky Way halo from galaxy kinematics
• Revealing strong bias in common measures of galaxy properties using new inclination-independent structures
• Exoplanets Across Galactic Stellar Populations with PLATO: Estimating Exoplanet Yields Around FGK Stars for the Thin Disk, Thick Disk and Stellar Halo
• Effect of orbital trapping by bar resonances in the local U-V velocity field
• Ripples spreading across the Galactic disc. Interplay of direct and indirect effects of the Sagittarius dwarf impact
• Metallicity Gradient of the Thick Disc Progenitor at High Redshift
• Stellar streams around the Magellanic Clouds in 4D
• A halo of trapped interstellar matter surrounding the solar system
• Testing a theoretical prediction for bar formation in galaxies with bulges
• On the Galactic rotation curve inferred from the Jeans equations Assessing its robustness using Gaia DR3 and cosmological simulations
• Dependence of Galactic Halo Kinematics on the Adopted Galactic Potential
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• Evidence of a Cloud-Cloud Collision from Overshooting Gas in the Galactic Center
• Towards a fully consistent Milky Way disk model -- IV. The impact of Gaia DR2 and APOGEE
• A giant galaxy in the young Universe with a massive ring
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Stellar encounters with giant molecular clouds
• Galactic Extinction: How Many Novae Does it Hide and How Does it Affect the Galactic Nova Rate?
• The Pristine Inner Galaxy Survey (PIGS) IV: A photometric metallicity analysis of the Sagittarius dwarf spheroidal galaxy
• Evidence that Mass Loss on the Red Giant Branch Decreases with Metallicity
• Searching for Milky Way twins: Radial abundance distribution as a strict criterion
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• Predicting the water content of interstellar objects from galactic star formation histories
• Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
• Vertical Structure and Kinematics of the Galactic Outer Disk
• Chemodynamical Analysis of Metal-rich High-eccentricity Stars in the Milky Way's Disk
• Solo dwarfs IV: Comparing and contrasting satellite and isolated dwarf galaxies in the Local Group
• Searching for a kinematic signature of the moderately metal-poor stars in the Milky Way bulge using N-body simulations
• A low density-wave spiral pattern speed, from the tracer separations (age gradient) across a spiral arm in the Milky Way
• Evidence For Multiple Accretion Events in the $Gaia$-Sausage/Enceladus Structures
• A Distant Sample of Halo Wide Binaries from SDSS
• The LMC impact on the kinematics of the Milky Way satellites: clues from the running solar apex
• Evidence for Populations-dependent vertical motions and the Long-lived Non-Steady Lopsided Milky Way Warp
• Geometric Aspects and Testing of the Galactic Center Distance Determination from Spiral Arm Segments
• The vertical metallicity gradients of mono-age stellar populations in the Milky Way with the RAVE and Gaia data
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• The spiral potential of the Milky Way
• Dark matter substructure cannot explain properties of the Fermi Galactic Centre excess
• Deceleration of kicked objects due to the Galactic potential
• A collage of small planets from the Lick Carnegie Exoplanet Survey : Exploring the super-Earth and sub-Neptune mass regime
• The Panchromatic Hubble Andromeda Treasury XX: The Disk of M31 is Thick
• Constraining the Milky Way's Ultraviolet to Infrared SED with Gaussian Process Regression
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Constraining Solar position and velocity with a Nearby Hypervelocity Star
• Growing the First Galaxies' Merger Trees
• Insights into the Formation and Evolution History of the Galactic Disk System
• OGLE-2016-BLG-1266: A Probable Brown-Dwarf/Planet Binary at the Deuterium Fusion Limit
• Robust Clustering of the Local Milky Way Stellar Kinematic Substructures with Gaia eDR3
• Disk flaring with TNG50: diversity across Milky Way and M31 analogs
• Weighing the IMBH candidate CO-0.40-0.22* in the Galactic Centre
• The local rotation curve of the Milky Way based on SEGUE and RAVE data
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• Beyond the Local Volume. II. Population Scaleheights and Ages of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
• Impact of bar resonances in the velocity-space distribution of the solar neighbourhood stars in a self-consistent $N$-body Galactic disc simulation
• A spectroscopic and kinematic survey of fast hot subdwarfs
• The binding of cosmological structures by massless topological defects
• Local clustering of relic neutrinos with kinetic field theory
• The Pristine survey -- XX: GTC follow-up observations of extremely metal-poor stars identified from Pristine and LAMOST
• Solar System Migration Points to a Renewed Concept: Galactic Habitable Orbits
• Dynamical evolution of Milky Way globular clusters on the cosmological timescale I. Mass loss and interaction with the nuclear star cluster
• Modelling mass distribution of the Milky Way galaxy using Gaia billion-star map
• Spatial and Kinematic Clustering of Stars in the Galactic Disk
• Characterising abundance-age relations of GALAH stars using oxygen-enhanced stellar models
• Applying Noether's theorem to matter in the Milky Way: evidence for external perturbations and non-steady-state effects from Gaia Data Release 2
• Efficient radial migration by giant molecular clouds in the first several hundred Myr after the stellar birth
• Photometric Signature of Ultra-Harmonic Resonances in Barred Galaxies
• The Chemical Composition of Extreme-Velocity Stars
• Exploring the Dust Content of Galactic Halos with Herschel. IV. NGC 3079
• Tracing Dark Matter Halos with Satellite Kinematics and the Central Stellar Velocity Dispersion of Galaxies
• Gemini/Phoenix H-band analysis of the globular cluster AL3
• Differential rotation of the halo traced by the K-giant stars
• Imprints of Zero-Age Velocity Dispersions and Dynamical Heating on the Age-Velocity dispersion Relation
• Turning up the heat on `Oumuamua
• Local Stellar Kinematics from RAVE data -- VIII. Effects of the Galactic Disc Perturbations on Stellar Orbits of Red Clump Stars
• A radiation transfer model for the Milky Way. II The global properties and large scale structure
• Drivers of disc tilting I: Correlations and possible drivers for Milky Way analogues
• Kerr-Newman black hole lensing of relativistic massive particles in the weak field limit
• Bar-driven dispersal of Galactic substructure
• Modeling Turbulence in Galactic Centers
• Milky Way globular clusters on cosmological timescales. III. Interaction rates
• 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
• The population of planetary nebulae near the Galactic centre: chemical abundances
• Two Populations of Carbon-Enhanced Metal-Poor Stars in the Disk System of the Milky Way
• Study of the Open Clusters in Kepler Prime Field
• High-Drag Interstellar Objects And Galactic Dynamical Streams
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Leading-order deflection of particles by a moving Schwarzschild lens with a two-dimensional velocity
• Census of Gaseous Satellites around Local Spiral Galaxies
• Milky Way globular clusters on cosmological timescales. II. Interaction with the Galactic centre
• Revealing Gas Inflows towards the Galactic Central Molecular Zone
• Populating The Milky Way: Characterising Planet Demographics by Combining Galaxy Formation Simulations and Planet Population Synthesis Models
• Jeans that fit: weighing the mass of the Milky Way analogues in the $\Lambda \mathrm{CDM}$ universe
• Exploring the impact of a rapidly decelerating bar on transforming bulge orbits into disc-like orbits
• Signatures of the Galactic bar on stellar kinematics unveiled by APOGEE
• Limits on dark matter annihilation in prompt cusps from the isotropic gamma-ray background
• Searching for Extragalactic Exoplanetary Systems: the Curious Case of BD+20 2457
• Primordial mass segregation of star clusters with primordial binaries
• Exploring Hydrodynamic Instabilities along the Infalling High-Velocity Cloud Complex A
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• Blanco DECam Bulge Survey (BDBS) V. Cleaning the foreground populations from Galactic bulge colour-magnitude diagrams using Gaia EDR3
• 3D Parameter Maps of Red Clump Stars in the Milky Way -- Absolute Magnitudes and Intrinsic Colors
• The Andromeda Gamma-Ray Excess: Background Systematics of the Millisecond Pulsars and Dark Matter Interpretations
• Zoom-in cosmological hydrodynamical simulation of a star-forming barred, spiral galaxy at redshift z=2
• Influence of the Galactic bar on the kinematics of the disc stars with Gaia EDR3 data
• Manifold spirals in barred galaxies with multiple pattern speeds
• Non-Parametric Spherical Jeans Mass Estimation with B-splines
• Reliable stellar abundances of individual stars with the MUSE integral-field spectrograph
• How well can we unravel the accreted constituents of the Milky Way stellar halo? A test on cosmological hydrodynamical simulations
• Galactic disc heating by density granulation in fuzzy dark matter simulations
• First spiral arm detection using dynamical mass measurements of the Milky Way disk
• Deep Potential: Recovering the gravitational potential from a snapshot of phase space
• Equilibrium axisymmetric halo model for the Milky Way and its implications for direct and indirect DM searches
• The dynamics of Galactic centre pulsars: constraining pulsar distances and intrinsic spin-down
• Benfords law in the Gaia universe
• Calibrating the BHB Star Distance Scale and the Halo Kinematic Distance to the Galactic Centre
• The Number of Possible CETIs within Our Galaxy and the Communication Probability among These CETIs
• The Density Profile and Kinematics of the Milky Way with RR Lyrae Stars
• A machine learning approach to photometric metallicities of giant stars
• Constraining the Milky Way Mass with Its Hot Gaseous Halo
• Understanding the velocity distribution of the Galactic Bulge with APOGEE and Gaia
• Precise distances from OGLE-IV member RR Lyrae stars in six bulge globular clusters
• North Polar Spur: gaseous plume(s) from star-forming regions at $\sim$3-5 kpc from Galactic Center?
• New classical Cepheids in the inner part of the northern Galactic disk and their kinematics
• The Galactic Bulge exploration IV.: RR~Lyrae stars as traces of the Galactic bar -- 3D and 5D analysis, extinction variation
• The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies
• Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc
• Predictions on the stellar-to-halo mass relation in the dwarf regime using the empirical model for galaxy formation EMERGE
• Rediscovering the Milky Way with orbit superposition approach and APOGEE data I. Method validation
• A non-axisymmetric potential for the Milky Way disk
• Quantifying torque from the Milky Way bar using Gaia DR2
• The Chemodynamics of the Stellar Populations in M31 from APOGEE Integrated Light Spectroscopy
• Comparison of the Stellar Populations of Bulges and Discs using the MaNGA Survey
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• Quantifying the influence of bars on action-based dynamical modelling of disc galaxies
• The Influence of the Galactic Bar on the Dynamics of Globular Clusters
• Deciphering the Milky Way disc formation time encrypted in the bar chrono-kinematics
• The GALAH Survey: Velocity fluctuations in the Milky Way using red clump giants
• On the Origin of High-velocity Clouds in the Galaxy
• Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE
• Trojan globular clusters: radial migration via trapping in bar resonances
• Chemodynamic evolution of Sun-like stars in nearby moving groups
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• A Blueprint for the Milky Way's Stellar Populations. V. 3D Local Dust Extinction
• Radial and azimuthal gradients of the moving groups in Gaia DR3: The slow/fast bar degeneracy problem
• Formation and evolution of the local interstellar environment: combined constraints from nucleosynthetic and X-ray data
• Voyage 2050 White Paper: All-Sky Visible and Near Infrared Space Astrometry
• A Catalog of Galactic Supernova Remnants and Supernova Remnant Candidates from the EMU/POSSUM Radio Sky Surveys. I
• Existence of the Metal-Rich Stellar Halo and High-velocity Thick Disk in the Galaxy
• Recommended conventions for reporting results from direct dark matter searches
• Element abundance analysis of the metal-rich stellar halo and high-velocitythick disk in the galaxy
• A Very Metal-poor RR Lyrae Star with a Disk Orbit Found in the Solar Neighborhood
• A catalogue of asteroseismically calibrated ages for APOGEE DR17. The predictions of a CatBoost machine learning model based on the [Mg/Ce] chemical clock and other stellar parameters
• The truncation of the disk of NGC 4565: Detected up to z=4 kpc, with star formation, and affected by the warp
• Observable Signatures of the Ejection Speed of Interstellar Objects from their Birth Systems
• Probing the Halo Gas Distribution in the Inner Galaxy with Fermi Bubble Observations
• Flipping of the tidal tails of the Ophiuchus stream due to the decelerating Galactic bar
• Stellar Streams in Chameleon Gravity
• Probing modified Newtonian dynamics with hypervelocity stars
• Formation rate of LB-1-like systems through dynamical interactions
• Millisecond Pulsar Kicks Cause Difficulties in Explaining the Galactic Center Gamma-Ray Excess
• Coronal Properties of Low-mass Population III Stars and the Radiative Feedback in the Early Universe
• A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematics
• Two substructures in the nearby stellar halo found in Gaia and RAVE
• Are Milky-Way-like galaxies like the Milky Way? A view from SDSS-IV/MaNGA
• The tilt of the velocity ellipsoid of different Galactic disk populations
• Exploring the ex-situ components within Gaia DR3
• LISA double white dwarf binaries as Galactic accelerometers
• The Gaia spectroscopic catalogue of exoplanets and host stars
• Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe
• Astrophysical signatures of leptonium
• Bar-spiral interaction produces radial migration and star formation bursts
• A method to calculate the local density distribution of the Galaxy from the Tycho-Gaia Astrometric Solution data
• Detecting Ultralight Dark Matter with Matter Effect
• Resolved Stellar Populations as Tracers of Outskirts
• Following the tidal trail: a history of modeling the Magellanic Stream
• Turbulent gas-rich discs at high redshift: origin of thick stellar discs through 3D 'baryon sloshing'
• The effect of our local motion on the Sandage-Loeb test of the cosmic expansion
• SSSpaNG! Stellar Spectra as Sparse, data-driven, Non-Gaussian processes
• A Galactic Self-Portrait: Density Structure and Integrated Properties of the Milky Way Disk
• Population synthesis of hot subdwarf B stars with COMPAS: on the observed Galactic population
• Insights into the physics when modeling cold gas clouds in a hot plasma
• Towards a fully consistent Milky Way disk model V. The disk model for 4 $-$ 14 kpc
• Dynamical streams in the local stellar halo
• GaiaUnlimited: The old stellar disc of the Milky Way as traced by the Red Clump
• Galaxy Zoo JWST: Up to 75% of discs are featureless at $3<z<7$
• First measurement of the triaxiality of the inner dark matter halo of the Milky Way
• Are the double-mode bulge RR Lyrae stars with identical period-ratios the relic of a disrupted stellar system?
• Axial Asymmetry Studies in Gaia Data Release 2 Yield the Pattern Speed of the Galactic Bar
• High Velocity Runaway Binaries from Supernovae in Triple Systems
• The GALAH Survey: Improving our understanding of confirmed and candidate planetary systems with large stellar surveys
• On the many '3-kiloparsec arms' - shocked wave and nuclear rotation
• The distribution, kinematics and luminosities of extreme helium stars as probes of their origin and evolution
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• New transient Galactic bulge intermediate polar candidate XMMU J175035.2-293557
• XENONnT WIMP Search: Signal & Background Modeling and Statistical Inference
• A mass-velocity anisotropy relation in galactic stellar disks
• Orientation of the spins of galaxies in the Local volume
• The New Astronomical Frontier of Interstellar Objects
• Decoding NGC 628 with radiative transfer methods
• Revealing the Milky Way's Most Recent Major Merger with a Gaia EDR3 Catalog of Machine-Learned Line-of-Sight Velocities
• A revised view of the Canis Major stellar overdensity with DECam and Gaia: new evidence of a stellar warp of blue stars
• Galactic Archeology with 4MOST
• Astrophysical Parameters and Dynamical Evolution of Open Clusters: NGC 2587, Col 268, Mel 72, Pismis 7
• Models of Bars with Exponential Density Profiles
• Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
• The bi-modal ${}^7$Li distribution of the Milky Way's thin-disk dwarf stars: The role of Galactic-scale events and stellar evolution
• SiO Maser Survey towards off-plane O-rich AGBs around the orbital plane of the Sagittarius Stellar Stream
• The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
• Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity
• Mapping the Milky Way in 5-D with 170 Million Stars
• Pairing function of visual binary stars
• Constraining Ultra Light Dark Matter with the Galactic Nuclear Star Cluster
• On the Origin of the Globular Cluster FSR 1758
• Through Thick and Thin: The Cosmic Evolution of Disk Scale Height
• AuriDESI: Mock Catalogues for the DESI Milky Way Survey
• The imprint of dark matter on the Galactic acceleration field
• Cluster membership analysis with supervised learning and $N$-body simulations
• Dynamical Friction due to fuzzy dark matter on satellites described by axisymmetric logarithmic potentials
• Prospects of newly detecting nearby star-forming galaxies by the Cherenkov Telescope Array
• Constraints on sub-terrestrial free-floating planets from Subaru microlensing observations
• Stellar Migration and Chemical Enrichment in the Milky Way Disc: A Hybrid Model
• Rediscovering the Galactic outer disk with LAMOST data
• The influence of dark matter halo on the stellar stream asymmetry via dynamical friction
• Gamma-ray and radio background constraints on cosmic rays in Milky Way circumgalactic medium
• Discovery of the shell structure via break radii in the outer halo of the Milky Way
• Rubin LSST observing strategies to maximize volume and uniformity coverage of Star Forming Regions in the Galactic Plane
• The Impact of Classical Bulges on Stellar Bars and Box-Peanut-X-Features in Disk Galaxies
• Turbulent Pressure Heats Gas and Suppresses Star Formation in Galactic Bar Molecular Clouds
• Galactic Stellar Populations from Photometric Metallicity Distribution Functions
• Gas Transfer Between the Inner 3-kpc Disk and the Galactic Central Molecular Zone
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
• Numerical Study of Statistical Properties of the Galactic Center Distance Estimate from the Geometry of Spiral Arm Segments
• The role of triple evolution in the formation of LISA double white dwarfs
• Water emission tracing active star formation from the Milky Way to high-$z$ galaxies
• The "Building Blocks" of Stellar Halos
• Study of the Influence of an Evolving Galactic Potential on the Orbital Properties of 152 Globular clusters with Data from the Gaia EDR3 Catalogue
• Cold-mode and hot-mode accretion in galaxy formation: an entropy approach
• Three-component Stackel model of the Galaxy based on the rotation curve from maser data
• Stellar evolution and modelling stars
• An astrometric and spectroscopic study of the $\delta$ Scuti variable HD21190 and its wide companion CPD -83${}^{\circ }$ 64B
• A Vertically Orientated Dark Matter Halo Marks a Flip of the Galactic Disk
• Can Thorne-$\dot{\text{Z}}$ytkow Objects source GW190814-type events?
• Galactic cartography with SkyMapper: I. Population sub-structure and the stellar number density of the inner halo
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• Probing the Scalar WIMP-Pion Coupling with the first LUX-ZEPLIN data
• Characterizing the Evolved Stellar Population in the Galactic Foreground I: Bolometric Magnitudes, Spatial Distribution and P-L Relations
• The Chemodynamical Nature of the Triangulum-Andromeda Overdensity
• The effect of kick velocities on the spatial distribution of millisecond pulsars and implications for the Galactic center excess
• Autonomous Gaussian decomposition of the Galactic Ring Survey. II. The Galactic distribution of 13CO
• Mysterious Globular Cluster System of the Peculiar Massive Galaxy M85
• Estimation of the Galactocentric Distance of the Sun from Cepheids Close to the Solar Circle
• Kinematic distinction of the two subpopulations of X-ray pulsars
• Milky Way globular clusters on cosmological timescales. IV. Guests in the outer Solar System
• Damping of the Milky Way bar by manifold-driven spirals
• Microlensing of dark matter models in the Milky Way
• Destruction of the central black hole gas reservoir through head-on galaxy collisions
• Tracing the Origins of Hot Halo Gas in Milky Way-Type Galaxies with SMUGGLE
• Detecting Interstellar Objects Through Stellar Occultations
• First resolved stellar halo kinematics of a MW-mass galaxy outside the Local Group: A flat counter-rotating halo in NGC 4945
• Linking high-z and low-z: Are We Observing the Progenitors of the Milky Way with JWST?
• An MCMC Approach to the Three-dimensional Structure of the Milky Way Bulge using OGLE-IV $\delta$ Scuti Stars
• Spectral Evidence of Solar Neighborhood Analogs in CALIFA Galaxies
• Detailed Mapping of the Galactic Disk Structure in the Solar Neighborhood through LAMOST K Dwarfs
• Cosmological implications of the Gaia Milky Way declining rotation curve
• Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary
• An analytic description of substructure-induced gravitational perturbations in stellar systems
• Dynamical evolution of the open clusters with different star formation efficiencies and orbital parameters
• Integrals of motion for non-axisymmetric potentials
• Very metal-poor stars in the solar vicinity: kinematics and abundance analysis
• Cosmological insights into the early accretion of r-process-enhanced stars II. Dynamical identification of lost members of Reticulum II
• SISSI: Supernovae in a stratified, shearing interstellar medium -- I. The geometry of supernova remnants
• Probabilistic galactic dynamics I - the Sun and GJ 710 with Monte Carlo, linearised and unscented treatments
• Cosmic-ray electrons and the magnetic field of the North Polar Spur
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Searching for new Hypervelocity Stars with Gaia DR3 and VLT/FORS2 Spectroscopy
• Line-of-sight mass estimator and the masses of the Milky Way and Andromeda Galaxy
• Gravitational deflection of light in polar-axis plane of a moving Kerr-Newman black hole
• Architecture of the Andromeda: a quantitative analysis of clustering in the inner stellar halo
• The 800pc long tidal tails of the Hyades star cluster: Possible discovery of candidate epicyclic overdensities from an open star cluster
• Using dust to constrain dark matter models
• Concerning the occurrence of bow shocks around high-mass X-ray binaries
• Variable stars in the northern Galactic plane from KISOGP
• The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk
• Semi-Analytic Modeling of Dark Matter Subhalo Encounters with Thin Stellar Streams: Statistical Predictions for GD-1-like Streams in CDM
• A proposal for enhancing technosignature search toward the Galactic center
• The DR14 APOGEE-TGAS catalogue: Precise chemo-kinematics in the extended solar vicinity
• The GECKOS Survey: Resolved, multiphase observations of mass-loading and gas density in the galactic wind of NGC 4666
• On the baryon budget in the X-ray-emitting circumgalactic medium of Milky Way-mass galaxies
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• Nuclear recoil response of liquid xenon and its impact on solar 8B neutrino and dark matter searches
• A search for photometric variability towards the globular cluster M3 with the TWenty Inch Survey Telescope
• A Preference for Cold Dark Matter over Superfluid Dark Matter in Local Milky Way Data
• An LBT view of the co-rotating group of galaxies around NGC 2750: Deep imaging and new satellite candidates
• Spatial mixing of stellar populations in globular clusters via binary-single star scattering
• Leptonic and hadronic models of high-energy nebula around V4641 Sgr
• The barred inner Milky Way: dynamical models from surveys
• Constraints On Covariant WIMP-Nucleon Effective Field Theory Interactions from the First Science Run of the LUX-ZEPLIN Experiment
• Signatures of simulated spiral arms on radial actions
• The highest mass Kepler red giants -- II. Spectroscopic parameters, the amplitude-activity relation, and unexpected halo orbits
• Stellar halo striations from assumptions of axisymmetry
• Comparing the structural parameters of the Milky Way to other spiral galaxies
• Influence of the Galactic gravitational field on the positional accuracy of extragalactic sources. II Observational appearances and detectability
• Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions
• Globular clusters as indicators of Galactic evolution
• Cosmic Rays and Non-thermal Emission Induced by Accretion of Cool Gas onto the Galactic Disk
• Supernova explosions of runaway stars and young neutron stars above the Galactic plane
• The mass-metallicity relation at z>3 down to M_*= 10^4 M_Sun. A local perspective using the metallicity distribution of RR Lyrae stars
• The Axial Zone of Avoidance in the Globular Cluster System and the Distance to the Galactic Center
• The Spheroidal Bulge of the Milky Way: Chemodynamically Distinct from the Inner-Thick Disc and Bar
• A Hint of Three-section Halo as Seen from the APOGEE DR14
• A long-lived compact jet in the black hole X-ray binary candidate AT2019wey
• UBVI CCD Photometry of Berkeley 55 Open Cluster
• A search for distant, pulsating red giants in the southern halo
• Outer Regions of the Milky Way
• Properties of Barred Galaxies with the Environment: II. The case of the Cosmic Web around the Virgo cluster
• Dissecting stellar populations with manifold learning I. Validation of the method on a synthetic Milky Way-like galaxy
• Leading-order gravitational time delay of massive particles by a moving Schwarzschild lens
• Modelling the Milky Way's exoplanet population based on cosmological galaxy simulations
• BASS. XLIV. Morphological preferences of local hard X-ray selected AGN
• NIHAO-LG: The uniqueness of Local Group dwarf galaxies
• The dark matter wake of a galactic bar revealed by multichannel Singular Spectral Analysis
• Stirring Things Up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue
• Classical Be Stars and Classical Be Star Binaries from LAMOST DR12
• HE0144-4657: A Carbon-Enhanced Ultra Metal-Poor Star ([Fe/H] ~ -4.1) from the Helmi Stream Disrupted Dwarf Galaxy
• Gravitational influence of the globular cluster NGC 7078 (M 15) flyby of the Oort cloud system
• Evidence of distant spiral arms in the Galactic disk quadrant IV from VVV red clump giants
• Threading the Magellanic Needle: Hypervelocity Stars Trace the Past Location of the LMC
• The Spiral Pattern Speed in the Milky Way Galaxy
• Astrophysical and Structural Parameters, And Dynamical Evolution Of The Open Clusters NGC 1245 And NGC 2099
• First large scale spatial and velocity patterns of local metal-rich stars in the Milky Way
• An Integral Field Spectroscopy Study Of Thin And Thick Discs In IC 2531
• The Magellanic Edges Survey -- II. Formation of the LMC's northern arm
• The Predicted Properties of Helium-Enriched Globular Cluster Progenitors at High Redshift
• Dynamical traction and black hole orbital migration
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
• Timing Mass of the Local Group
• Large-Scale Surveys of Pulsating Stars for Studying Stellar Populations in the Inner Galaxy
• Eikonal gravitational-wave lensing in Einstein-aether theory
• Milky Way Mass Through Escape Velocity Curve from LAMOST K Giants
• The survey of Planetary Nebulae in Andromeda (M31): I. Imaging the disk and halo with MegaCam@CFHT
• Using N-body simulations to understand the chemo-dynamical evolution of the inner Milky Way
• Towards Understanding the Milky Way's Typicality: Assessing the Chemodynamics of M31's Bulge & Bar, Thick & Thin Discs
• Modeling the vertical distribution of the Milky Way's flat subsystem objects
• Study of Galactic Structure Using UVIT/AstroSat Star Counts
• Calibrating the Color-Magnitude Relation of M Giants by Using Open Clusters
• The Baryonic Mass Estimates of the Milky Way Halo in the form of High Velocity Clouds
• Asteroseismology of red giants & galactic archaeology
• Searching for stars ejected from the Galactic Centre in DESI
• 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
• A hierarchical clustering method for quantifying satellite abundance
• Solar twins in Gaia DR3 GSP-Spec II. Age distribution and its implications for the Sun's migration
• X-ray emission of the Nuclear Stellar Disk as seen by SRG/ART-XC
• Kinematics of the Milky way from the statistical analysis of the Gaia Data Release 3
• Spatially Resolved Properties of Extraplanar Diffuse Ionized Gas in NGC3511 and NGC3513
• Bar Properties and Star-by-Star Bar Membership via Action Conservation
• On the possible orbital motion of Sgr A* in the smooth potential of the Milky Way
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Close Encounters of the Interstellar Kind: Examining the Capture of Interstellar Objects in Near Earth Orbit
• Dynamical properties of high-[Mg/Fe] stars in the Milky Way bar region
• Fast radio bursts by stellar wind microlensing of a faint background source
• Search for Galactic warp signal in Gaia DR1 proper motions
• Supergiant GCIRS 22 in the Milky Way Nuclear Star Cluster: Revised alpha abundances
• How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• Beyond LCDM: Bits join the Dark Side
• A family of potential-density pairs for galactic bars
• Infrared photometry and CaT spectroscopy of the most metal-poor in-situ globular cluster VVV-CL001
• Diffuse Hot Plasma in the Interstellar Medium and Galactic Outflows
• Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey
• The Baryonic Tully-Fisher Relation in the Local Group and the Equivalent Circular Velocity of Pressure Supported Dwarfs
• Distance and extinction to the Milky Way spiral arms along the Galactic centre line of sight
• Metallicity Structure in Galactic Longitude-Velocity Diagrams of the Milky Way Disk and FIRE-2 Simulations
• The Exploration of Local VolumE Satellites (ELVES) Survey: A Nearly Volume-Limited Sample of Nearby Dwarf Satellite Systems
• Neutron-capture elements record the ordered chemical evolution of the disc over time
• A Tilt in the Dark Matter Halo of the Galaxy
• Strong field gravitational lensing of particles by a black-bounce-Schwarzschild black hole
• Improved constraints on modified Newtonian gravity from Cassini radio tracking data
• The HaloSat and PolarLight CubeSat Missions for X-ray Astrophysics
• Selecting Post-Starburst Galaxies Based on Star Formation History
• Projected Sensitivity of Paleo-Detectors to Dark Matter Effective Interactions with Nuclei
• On the detection of stellar wakes in the Milky Way: a deep learning approach
• Rapid early gas accretion for the inner Galactic disc
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• The multiple corrugations in the Galactic disk derived from the LAMOST and Gaia survey data
• A Dynamical Evolution Study of the Open Clusters: Berkeley 10, Berkeley 81, Berkeley 89 and Ruprecht 135
• Spectroscopic analysis of VVV CL001 cluster with MUSE
• A Kinematically Cold Structure of Candidate Young OB Stars Toward The Anticenter
• A comparative study of O, Ne, Cl, and Ar in Hii regions and PNe of the Galactic disk: Temporal evolution of radial gradients?
• Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data
• Assessing the Impact of Hydrogen Absorption on the Characteristics of the Galactic Center Excess
• Self-consistent modelling of the Milky Way's Nuclear Stellar Disc
• J-PLUS Reconstructing the Milky Way Disc's star formation history with twelve-filter photometry
• Turning Points in the Age-Metallicity Relations -- Created by Late Satellite Infall and Enhanced by Radial Migration
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Intrinsic properties of the bars formed by the bar instability in flat stellar discs
• Chemo-dynamical abundance analysis of the very metal-poor halo star HE 2315-4240
• CCD UBVRI photometry of the open cluster Berkeley 8
• The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
• SCF-FDPS: A Fast $N$-body Code for Simulating Disk-halo Systems
• An ancient system hidden in the Galactic plane?
• Insights into the structure and kinematics of a Milky Way-like galaxy
• Understanding the Galaxy
• Age distribution of stars in boxy/peanut/X-shaped bulges formed without bar buckling
• The dynamical state of bars in cluster dwarf galaxies: The cases of NGC 4483 and NGC 4516
• Dynamical Evolution of The Open Clusters Collinder 110 and NGC 2477