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