The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems

Abstract

The distribution of stellar masses that form in one star-formation event in a given volume of space is called the initial mass function (IMF). The IMF has been estimated from low-mass brown dwarfs to very massive stars. Combining IMF estimates for different populations in which the stars can be observed individually unveils an extraordinary uniformity of the IMF. This general insight appears to hold for populations including present-day star formation in small molecular clouds, rich and dense massive star-clusters forming in giant clouds, through to ancient and metal-poor exotic stellar populations that may be dominated by dark matter. This apparent universality of the IMF is a challenge for star formation theory because elementary considerations suggest that the IMF ought to systematically vary with star-forming conditions.

32 pages, all 6 figures are in colour, published in Science

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• On The Nature of Variations in the Measured Star Formation Efficiency of Molecular Clouds
• Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies
• Astrometric and photometric initial mass functions from the UKIDSS Galactic Clusters Survey: I The Pleiades
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• Looking into the hearts of Bok globules: MM and submm continuum images of isolated star-forming cores
• The Star Formation History and Dust Content in the Far Outer Disc of M31
• The brightest stars of the sigma Orionis cluster
• On the fraction of intermediate-mass close binaries that explode as type-Ia supernovae
• The Evolution of the Star Formation Rate of Galaxies at 0.0 < z < 1.2
• Does the dwarf galaxy system of the Milky Way originate from Andromeda?
• The Starburst Cluster Westerlund 1: The Initial Mass Function and Mass Segregation
• The building up of the disk galaxy M33 and the evolution of the metallicity gradient
• Combining Stellar Populations with Orbit-Superposition Dynamical Modelling - the Formation History of the Lenticular Galaxy NGC 3115
• Formation of Ultracompact X-ray Binaries in Dense Star Clusters
• Impact of the cosmic background radiation on the initial mass function of metal-poor stars
• The Stellar Mass Spectrum in Warm and Dusty Gas: Deviations from Salpeter in the Galactic Centre and in Circum-Nuclear Starburst Regions
• Unbound Young Stellar Systems: Star Formation on the loose
• Stellar population of the superbubble N206 in the LMC II. Parameters of the OB and WR stars, and the total massive star feedback
• Acceleration of ultrahigh-energy cosmic rays in starburst superwinds
• Evidence of a non universal stellar Initial Mass Function. Insights from HST optical imaging of 6 Ultra Faint Dwarf Milky Way Satellites
• Ultra-Deep Hubble Space Telescope Imaging of the Small Magellanic Cloud: The Initial Mass Function of Stars with M <~ 1 Msun
• The dynamics and star-forming potential of the massive Galactic centre cloud G0.253+0.016
• Prospects for chemically tagging stars in the Galaxy
• The influence of multiple stars on the high-mass stellar initial mass function and age-dating of young massive star clusters
• ALMA observations of 99 GHz free-free and H40$\alpha$ line emission from star formation in the centre of NGC 253
• Massive Outflows Driven by Magnetic Effects in Star Forming Clouds with High Mass Accretion Rates
• Low-Mass X-ray Binaries and Globular Clusters in Early-Type Galaxies. I. Chandra Observations
• Interacting supernovae and supernova impostors. LSQ13zm: an outburst heralds the death of a massive star
• Draco -- A Failure of the Tidal Model
• Powderday: Dust Radiative Transfer for Galaxy Simulations
• Carbon-Enhanced Metal-Poor Stars, the Cosmic Microwave Background, and the Stellar IMF in the Early Universe
• Internal dynamics and stellar content of nine ultra-diffuse galaxies in the Coma cluster prove their evolutionary link with dwarf early-type galaxies
• Simulating Star Clusters Across Cosmic Time: I. Initial Mass Function, Star Formation Rates and Efficiencies
• Likely Members of the Beta Pictoris and AB Doradus Moving Groups in the North
• The Metallicity Dependence of the Minimum Mass for Core-Collapse Supernovae
• A Catalog of Diffuse X-ray-Emitting Features within 20 pc of Sgr A*: Twenty Pulsar Wind Nebulae?
• Triggered Star Formation and Evolution of T-Tauri stars in and around Bright-Rimmed Clouds
• Dynamical Mass Estimates for Five Young Massive Stellar Clusters
• The Necessity of Feedback Physics in Setting the Peak of the Initial Mass Function
• Quenching timescales of dwarf satellites around Milky Way-mass hosts
• Zooming in on Individual Star Formation: Low- and High-mass Stars
• Kinematics of OB-associations in Gaia epoch
• A census of very-low-mass stars and brown dwarfs in the sigma Orionis cluster
• Resolving The Generation of Starburst Winds in Galaxy Mergers
• Characterizing the Brown Dwarf Formation Channels from the Initial Mass Function and Binary-star Dynamics
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• Age and Mass for 920 LMC Clusters Derived from 100 Million Monte Carlo Simulations
• Cluster dynamics largely shapes protoplanetary disc sizes
• Age spread in W3 Main: LBT/LUCI near-infrared spectroscopy of the massive stellar content
• Disk Evolution in OB Associations - Deep Spitzer/IRAC Observations of IC 1795
• S-Type and P-Type Habitability in Stellar Binary Systems: A Comprehensive Approach. I. Method and Applications
• Resolved photometry of extragalactic young massive star clusters
• Dynamics versus structure: breaking the density degeneracy in star formation
• The evolution of binary populations in cool, clumpy star clusters
• When the Jeans don't fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies
• Carbon-Enhanced Hyper-metal-poor Stars and the Stellar IMF at Low Metallicity
• On mini-halo encounters with stars
• Maximum stellar mass versus cluster membership number revisited
• The Formation of Star Clusters II: 3D Simulations of Magnetohydrodynamic Turbulence in Molecular Clouds
• Outflows, Accretion, and Clustered Protostellar Cores around a Forming O Star
• New low-mass members of the Octans stellar association and an updated 30-40 Myr lithium age
• Boötes IV: A New Milky Way Satellite Discovered in the Subaru Hyper Suprime-Cam Survey and Implications for the Missing Satellite Problem
• Cluster kinematics and stellar rotation in NGC 419 with MUSE and adaptive optics
• Generation of highly inclined protoplanetary discs through single stellar flybys
• Evidence for feedback and stellar-dynamically regulated bursty star cluster formation: the case of the Orion Nebula Cluster
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• GLIMPSE-CO1: the most massive intermediate-age stellar cluster in the Galaxy
• The Fornax 3D project: a two-dimensional view of the stellar initial mass function in the massive lenticular galaxy FCC 167
• The structure of molecular clouds and the universality of the clump mass function
• Dense Molecular Gas: A Sensitive Probe of Stellar Feedback Models
• Gravitational instability in protostellar disks at low metallicities
• The Complete Initial Mass Function Down to the Sub-Solar Regime in the Large Magellanic Cloud with Hubble Space Telescope ACS Observations
• SDSS-IV MaNGA: Spatially resolved star formation in barred galaxies
• Testing the universality of the IMF with Bayesian statistics: young clusters
• On the formation of very metal-poor stars: The case of SDSS J1029151+172927
• The initial conditions of star formation VIII: an observational study of the Ophiuchus cloud L1688 and implications for the prestellar core mass function
• Astrometric and photometric initial mass functions from the UKIDSS Galactic Clusters Survey: IV Upper Sco
• On the recent star formation history of the Milky Way disk
• Extreme chemical abundance ratio suggesting an exotic origin for an ultra-diffuse galaxy
• Coronae in the Coronet: A very deep X-ray look into a stellar nursery
• Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
• A simple method to convert sink particles into stars
• Stellar contents and star formation in the young open cluster Stock 8
• High Mass Star Formation. II. The Mass Function of Submillimeter Clumps in M17
• An Initial Mass Function for Individual Stars in Galactic Disks: I. Constraining the Shape of the IMF
• The Detailed Chemical Properties of M31 Star Clusters I. Fe, Alpha and Light Elements
• Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
• The Elephant Trunk Nebula and the Trumpler 37 cluster: Contribution of triggered star formation to the total population of an HII region
• Core Mass Function: The Role of Gravity
• The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev-Zel'dovich effect and soft X-ray emission
• The influence of gas expulsion and initial mass-segregation on the stellar mass-function of globular star clusters
• The star formation efficiency and its relation to variations in the initial mass function
• The temporal and spatial evolution of the starburst in ESO 338-IG04 as probed by its star clusters
• The IMF of stellar clusters: effects of accretion and feedback
• The Star Formation History in The Far Outer Disc of M33
• Brown dwarf formation by binary disruption
• Gas accretion from minor mergers in local spiral galaxies
• Is the Initial Mass Function of Low Surface Brightness Galaxies Dominated by Low Mass Stars?
• Cluster assembly and the origin of mass segregation in the STARFORGE simulations
• Spatially resolved variations of the IMF mass normalisation in early-type galaxies as probed by molecular gas kinematics
• A Cross-Match of 2MASS and SDSS. II. Peculiar L Dwarfs, Unresolved Binaries, and the Space Density of T Dwarf Secondaries
• Metallicity-dependendent kinematics and morphology of the Milky Way bulge
• A large moving group within the Lower Centaurus Crux association
• The resolved stellar populations around 12 Type IIP supernovae
• Supernova enrichment and dynamical histories of solar-type stars in clusters
• S-stars in the Galactic center and hypervelocity stars in the Galactic halo: two faces of the tidal breakup of stellar binaries by the central massive black hole?
• Further evidence for a time-dependent initial mass function in massive early-type galaxies
• Anatomy of a Young Massive Star Cluster: NGC 1569-B
• The fundamental gas depletion and stellar-mass buildup times of star forming galaxies
• On the formation of trapezium-like systems
• The Universal Initial Mass Function In The XUV Disk of M83
• Stellar Mass Spectra from Non-Isothermal Gravoturbulent Fragmentation
• Stellar contents and star formation in the young star cluster Be 59
• A Relationship Between Stellar Metallicity Gradients and Galaxy Age in Dwarf Galaxies
• JWST reveals a possible $z\sim 11$ galaxy merger in triply-lensed MACS0647$-$JD
• High Mass Star Formation. III. The Functional Form of the Submillimeter Clump Mass Function
• Fragmentation and Evolution of Molecular Clouds. II: The Effect of Dust Heating
• Star Formation at Very Low Metallicity. IV. Fragmentation Does Not Depend on Metallicity for Cold Initial Conditions
• Virgo Cluster and field dwarf ellipticals in 3D - II. Internal dynamics points to tidal harassment?
• Swirls of FIRE: Spatially Resolved Gas Velocity Dispersions and Star Formation Rates in FIRE-2 Disk Environments
• On the Origin of Diffuse Ionized Gas in the Antennae Galaxy
• Candidate Tidal Dwarf Galaxies in Arp 305: Lessons on Dwarf Detachment and Globular Cluster Formation
• The most massive stars in very young star clusters with a limited mass: Evidence favours significant self-regulation in the star formation processes
• Microlensing constraints on the Galactic Bulge Initial Mass Function
• Star formation in bright-rimmed clouds and cluster associated with W5 E H{\sc ii} region
• Spatial dependence of the Star Formation History in the Central Regions of the Fornax Dwarf Spheroidal Galaxy
• Confrontation of MOND Predictions with WMAP First Year Data
• The Initial Mass Function and Young Brown Dwarf Candidates in NGC 2264. IV. The Initial Mass Function and Star Formation History
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• Feedback regulated star formation: II. dual constraints on the SFE and the age spread of stars in massive clusters
• Star formation in the massive cluster merger Abell 2744
• Cool Companions to White Dwarfs from the 2MASS Second Incremental Data Release
• The Effect of Star Formation History on the Inferred Initial Stellar Mass Function
• The Fornax 3D project: Thick disks in a cluster environment
• On the origin of the Galactic thin and thick discs, their abundance gradients and the diagnostic potential of their abundance ratios
• Influence of primordial magnetic fields on 21 cm emission
• What Physics Determines the Peak of the IMF? Insights from the Structure of Cores in Radiation-Magnetohydrodynamic Simulations
• Chemo-dynamical evolution of tidal dwarf galaxies. I. Method and IMF dependence
• A quartet of black holes and a missing duo: probing the low-end of the Mbh - sigma relation with the adaptive optics assisted integral-field spectroscopy
• Mass functions and photometric binaries in nine open clusters
• Connection between dynamically derived IMF normalisation and stellar population parameters
• MASSCLEANage -- Stellar Cluster Ages from Integrated Colors --
• Finding Black Holes with Microlensing
• Evolution of giant molecular clouds across cosmic time
• Continuous star formation in IZw18
• The white dwarf luminosity function
• The very low-mass stellar content of the young supermassive Galactic star cluster Westerlund 1
• Close Binary Interactions of Intermediate-Mass Black Holes: Possible Ultra-Luminous X-ray Sources?
• Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies
• The metallicity distribution of the halo and the satellites of the Milky way in the hierarchical merging paradigm
• Appreciating mergers for understanding the non-linear $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ and $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{galaxy}}$ relations, updated herein, and the implications for the (reduced) role of AGN feedback
• Supernova dust formation and the grain growth in the early universe: The critical metallicity for low-mass star formation
• On the Evolution of the Dense Core Mass Function
• Realistic modeling of wind and supernovae shocks in star clusters: addressing ${}^{22}\mathrm{Ne}{/}^{20}\mathrm{Ne}$ and other problems in Galactic cosmic rays
• Mapping the core mass function to the initial mass function
• The Premature Formation of High Redshift Galaxies
• Internal motions in OB-associations with Gaia DR2
• Testing galaxy formation models with the GHOSTS survey: The color profile of M81's stellar halo
• The Origin of the Stellar Mass Distribution and Multiplicity
• Metallicity and the Universality of the IMF
• The Low-redshift Lyman-continuum Survey: [S II]-deficiency and the leakage of ionizing radiation
• Top-heavy integrated galactic stellar initial mass functions (IGIMFs) in starbursts
• The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
• Trapping of HII regions in Population III star formation
• On the spatial distribution and the origin of hypervelocity stars
• The Galactic Dust-Up: Modeling Dust Evolution in FIRE
• The evolution of the binary population in globular clusters: a full analytical computation
• Detection of Ks-excess stars in the 14Myr open cluster NGC4755
• Rapid Evolution of the Innermost Dust Disk of Protoplanetary Disks Surrounding Intermediate-mass Stars
• S-Type and P-Type Habitability in Stellar Binary Systems: A Comprehensive Approach. II. Elliptical Orbits
• Multiple stellar populations in NGC 1866. New clues from Cepheids and Colour-Magnitude Diagram
• No evidence of mass segregation in the low mass Galactic globular cluster NGC 6101
• The Magellanic Bridge cluster NGC 796: Deep optical AO imaging reveals the stellar content and initial mass function of a massive open cluster
• A Method for Measuring Variations in the Stellar Initial Mass Function
• The Cosmic Timeline Implied by the JWST High-redshift Galaxies
• An X-ray census of young stars in the Chamaeleon I North cloud
• The Star Formation History of M32
• A New Brown Dwarf Desert? A Scarcity of Wide Ultracool Binaries
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• Interpreting the Colour-Magnitude Diagrams of Open Star Clusters through Numerical Simulations
• The stellar Initial Mass Function of the solar neighbourhood revealed by Gaia
• A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2
• An explanation for metallicity effects on X-ray Binary properties
• A first constraint on the average mass of ultra diffuse galaxies from weak gravitational lensing
• ALMA-IMF VI -- Investigating the origin of stellar masses: Core mass function evolution in the W43-MM2&MM3 mini-starburst
• The Identification of a Dusty Multiarm Spiral Galaxy at $z=3.06$ with JWST and ALMA
• Chemical evolution of ultra-faint dwarf galaxies in the self-consistently calculated IGIMF theory
• The Dynamical Fate of Self-Gravitating Disc Fragments After Tidal Downsizing
• Low Mass X-ray Binaries and Metallicity Dependence: Story of Failures
• Cosmological Implications of a Stellar Initial Mass Function that Varies with the Jeans Mass in Galaxies
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• Constraining the low-mass end of the Initial Mass Function with Gravitational Lensing
• Competitive feedback in galaxy formation
• The Close Companion Mass-Ratio Distribution of Intermediate-Mass Stars
• Resolved magnetic structures in the disk-halo interface of NGC 628
• The impact of stripped Nuclei on the Super-Massive Black Hole number density in the local Universe
• Mass-loss and expansion of ultra compact dwarf galaxies through gas expulsion and stellar evolution for top-heavy stellar initial mass functions
• WARPFIELD-EMP: The Self-Consistent Prediction of Emission Lines from Evolving HII Regions in Dense Molecular Clouds
• The binary companion mass ratio distribution: an imprint of the star formation process?
• Ages and metallicities of circumnuclear star formation regions from Gemini IFU observations
• Stochastic `Beads on a String' in the Accretion Tail of Arp 285
• Protostar Mass Due to Infall and Dispersal
• Accretion Does Not Drive the Turbulence in Galactic Disks
• Integral Field Spectroscopy of HII region complexes. The outer disk of NGC 6946
• Encounter-driven accretion in young stellar clusters - A connection to FUors?
• The chemical evolution of galaxies with a variable IGIMF
• On the mass segregation of stars and brown dwarfs in Taurus
• A rumble in the dark: signatures of self-interacting dark matter in Super-Massive Black Hole dynamics and galaxy density profiles
• The Hercules-Lyra Association revisited New age estimation and multiplicity study
• Metals and dust content across the galaxies M101 and NGC 628
• Herschel far-infrared observations of the Carina Nebula complex II: The embedded young stellar and protostellar population
• Protoplanetary Disk Evolution around the Triggered Star Forming Region Cepheus B
• The binary fraction in the globular cluster M10 (NGC 6254): comparing core and outer regions
• The Initial Mass Function and the Surface Density Profile of NGC 6231
• The bursty star formation history of the Fornax dwarf spheroidal galaxy revealed with the HST
• Joint constraints on the Galactic dark matter halo and Galactic Centre from hypervelocity stars
• Hierarchical star formation across the grand design spiral NGC1566
• The same, but different: Stochasticity in binary destruction
• An explanation for the unusual IMF in Taurus
• A WISE View of Star Formation in Local Galaxy Clusters
• Hierarchical Stellar Structures in the Local Group Dwarf Galaxy NGC 6822
• Super-star clusters versus OB associations
• Integrated Light Chemical Tagging Analyses of Seven M31 Outer Halo Globular Clusters from the Pan-Andromeda Archaeological Survey
• Astrometric and photometric initial mass functions from the UKIDSS Galactic Clusters Survey: III Praesepe
• Star Formation in the Bullet Cluster I: The Infrared Luminosity Function and Star Formation Rate
• A multi-wavelength view of cooling vs. AGN heating in the X-ray luminous cool-core of Abell 3581
• Reconstructing the Arches I: Constraining the Initial Conditions
• On the distribution of protostar masses
• The star formation history of the Sextans dwarf spheroidal galaxy: a true fossil of the pre-reionization era
• The Formation of Solar System Analogs in Young Star Clusters
• Stochastic Chemical Evolution of Galactic Subhalos and the Origin of r-Process Elements
• The stellar population and initial mass function of NGC 1399 with MUSE
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• The star formation history of the Sculptor dwarf spheroidal galaxy
• Breaking a dark degeneracy: The gamma-ray signature of early matter domination
• Filamentary condensations in a young cluster
• Characterizing Extreme Emission Line Galaxies II: A Self-Consistent Model of Their Ionizing Spectrum
• Globular Cluster Abundances from High-Resolution, Integrated-Light Spectroscopy. III. The Large Magellanic Cloud: Fe and Ages
• MODEST-1: Integrating Stellar Evolution and Stellar Dynamics
• Simulations of the Hyades
• High spatial resolution mid-infrared spectroscopy of NGC 5253: The stellar content of the embedded super-star cluster
• The young stellar population of NGC 4214 as observed with HST. II. Results
• Shock interactions, turbulence, and the origin of the stellar mass spectrum
• A complete census of Herschel-detected infrared sources within the HST Frontier Fields
• Free-free and H42alpha emission from the dusty starburst within NGC 4945 as observed by ALMA
• Star Formation in Molecular Clouds
• A Chandra Study of the Rosette Star-Forming Complex. II. Clusters in the Rosette Molecular Cloud
• Star formation in W3 - AFGL333: Young stellar content, properties and roles of external feedback
• The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
• The multiplicity fraction in 202 open clusters from Gaia
• Close Stellar Encounters in Young, Substructured, Dissolving Star Clusters: Statistics and Effects on Planetary Systems
• How do disks and planetary systems in high-mass open clusters differ from those around field stars?
• The Initial Mass Function of the Stellar Association NGC 602 in the Small Magellanic Cloud with Hubble Space Telescope ACS Observations
• On the halo-mass and radial scale dependence of the lensing is low effect
• Direct $N$-body simulations of globular clusters - II. Palomar 4
• The stellar contents and star formation in the NGC 7538 region
• Accretion bursts in young stars driven by cluster environment
• The Fornax3D project: Assembly histories of lenticular galaxies from a combined dynamical and population orbital analysis
• Evolution of the binary population in young dense star clusters
• Structure and kinematics of edge-on galaxy discs -- IV. The kinematics of the stellar discs
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• Bursting Bubbles: Feedback from Clustered SNe and the Trade-off Between Turbulence and Outflows
• The Complexity of the Cetus Stream Unveiled from the Fusion of STREAMFINDER and StarGO
• Local Luminous Infrared Galaxies. III. Co-evolution of Black Hole Growth and Star Formation Activity?
• A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations
• An Introduction to Galactic Chemical Evolution
• Wide binaries in ultra-faint galaxies: a window onto dark matter on the smallest scales
• Optical photometric and polarimetric investigation of NGC 1931
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• Star-forming accretion flows and the low luminosity nuclei of giant elliptical galaxies
• Population III Star Formation In Large Cosmological Simulations I. Halo Temporal and Physical Environment
• On the infant weight loss of low- to intermediate-mass star clusters
• Multiple Star Systems in the Orion Nebula
• Discovering young stars in the Gum 31 region with infrared observations
• The AMBRE project: a study of Li evolution in the Galactic thin and thick discs
• Constraints on the star formation history of the Large Magellanic Cloud
• Molecular Cloud-scale Star Formation in NGC 300
• Merger traces in the spatial distribution of stellar populations in the Fornax dSph galaxy
• Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales
• The Panchromatic Hubble Andromeda Treasury IV. A Probabilistic Approach to Inferring the High Mass Stellar Initial Mass Function and Other Power-law Functions
• Spectroscopy of Hyades L dwarf candidates
• The Binary Populations of Eight Globular Clusters in the Outer Halo of the Milky Way
• Modest-2: A Summary
• MASSCLEAN - MASSive CLuster Evolution and ANalysis Package - Description and Tests
• The statistical challenge of constraining the low-mass IMF in Local Group dwarf galaxies
• The galactocentric radius dependent upper mass limit of young star clusters: stochastic star formation ruled out
• Can magnetized turbulence set the mass scale of stars?
• First T dwarfs in the VISTA Hemisphere Survey
• Habitability around F-type Stars
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• Modelling mass distribution in elliptical galaxies: mass profiles and their correlation with velocity dispersion profiles
• Dynamical Mass Estimates for Two Luminous Young Stellar Clusters in Messier 83
• On the Age and Metallicity Estimation of Spiral Galaxies Using Optical and Near-Infrared Photometry
• On the Recovery of the Star Formation History of the LMC from the VISTA Survey of the Magellanic System
• Neutron star mergers as the astrophysical site of the r-process in the Milky Way and its satellite galaxies
• Measuring the Clump Mass Function in the Age of SCUBA2, Herschel, and ALMA
• Structure and Fragmentation of a high line-mass filament: Nessie
• The M/L ratio of massive young clusters
• The ACS Nearby Galaxy Survey Treasury IV. The Star Formation History of NGC 2976
• The MLP Distribution: A Modified Lognormal Power-Law Model for the Stellar Initial Mass Function
• The Hot, Accreted Halo of NGC 891
• Star formation in dense clusters
• The low-mass population in the young cluster Stock 8: Stellar properties and Initial Mass Function
• Shock generated vorticity in the interstellar medium and the origin of the stellar initial mass function
• Population Synthesis Models Indicate a Need for Early and Ubiquitous Disk Substructures
• Infrared High-Resolution Integrated Light Spectral Analyses of M31 Globular Clusters from APOGEE
• The M31 microlensing event WeCAPP-GL1/Point-AGAPE-S3: evidence for a MACHO component in the dark halo of M31?
• A comprehensive comparison of the Sun to other stars: searching for self-selection effects
• Mass and luminosity evolution of young stellar objects
• Flipping spins in mass transferring binaries and origin of spin-orbit misalignment in binary black holes
• Detecting Dark Matter Cores in Galaxy Clusters with Strong Lensing
• On the fidelity of the core mass functions derived from dust column density data
• The star formation history of the Large Magellanic Cloud star clusters NGC1846 and NGC1783
• The Astro-Primordial Black Hole Merger Rates: a Reappraisal
• One of the most massive stars in the Galaxy may have formed in isolation
• The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies
• MASSCLEANcolors - Mass Dependent Integrated Colors for Stellar Clusters Derived from 30 Million Monte Carlo Simulations -
• Habitability of Super-Earth Planets around Main-Sequence Stars including Red Giant Branch Evolution: Models based on the Integrated System Approach
• The Effect of Environment on Discs and Bulges
• The state of globular clusters at birth: emergence from the gas-embedded phase
• Globular Cluster Abundances from High-Resolution, Integrated-Light Spectroscopy. II. Expanding the Metallicity Range for Old Clusters and Updated Analysis Techniques
• A detailed study of the main sequence of the Globular Cluster NGC 6397: can we derive constraints on the existence of multiple population?
• The time evolution of the Milky Way's oxygen abundance gradient
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• The Pristine Inner Galaxy Survey (PIGS) III: carbon-enhanced metal-poor stars in the bulge
• Return of the TEDI: revisiting the Triple Evolution Dynamical Instability channel in triple stars
• Formation of the first stars
• A Galactic survey of radio jets from massive protostars
• The red supergiants & Wolf-Rayet stars of NGC 604
• Surface convection and red giants radii measurements
• The ISLANDS project I: Andromeda XVI, An Extremely Low Mass Galaxy not Quenched by Reionization
• Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
• The role of cluster evolution in disrupting planetary systems and disks: the Kozai mechanism
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• The disintegrating old open cluster Czernik 3
• The Sample of Red Supergiants in Twelve Low-Mass Galaxies of the Local Group
• A statistical view on stable and unstable Roche lobe overflow of a tertiary star onto the inner binary in triple systems
• The Fornax3D project: discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427
• Early evolutionary tracks of low-mass stellar objects in modified gravity
• The Gaia-ESO Survey: detection and characterization of single line spectroscopic binaries
• Sampling methods for stellar masses and the mmax-Mecl relation in the starburst dwarf galaxy NGC 4214
• Transforming gas-rich low-mass disky galaxies into ultra-diffuse galaxies by ram pressure
• Formation of proto-clusters and star formation within clusters: apparent universality of the initial mass function ?
• Galactic synchrotron emission and the FIR-radio correlation at high redshift
• The influence of stellar-dynamical ejections and collisions on the relation between the maximum-star and star-cluster-mass
• Chemical evolution of elliptical galaxies with a variable IMF -- A publicly available code
• Massive Stars: Their Birth Sites and Distribution
• Comparison of Theoretical Starburst Photoionisation Models for Optical Diagnostics
• Disentangling the metallicity and star formation history of HII galaxies through tailor-made models
• The stellar initial mass function at 0.9<z<1.5
• Stellar Stream and Halo Structure in the Andromeda Galaxy From a Subaru/Hyper Suprime-Cam Survey
• NICMOS/HST Observations of the Embedded Cluster Associated with Mon R2: Constraining the sub-stellar Initial Mass Function
• Planetary mass function and planetary systems
• A probabilistic analysis of the Fermi paradox in terms of the Drake formula: the role of the L factor
• Self-consistent Color-Mass-to-Light-Ratio relations for Low Surface Brightness Galaxies
• Is it possible to reconcile extragalactic IMF variations with a universal Milky Way IMF?
• Proper motion measurements as indicators of binarity in open clusters
• Masses and radii of four very low mass stars in F+M eclipsing binary systems
• The initial mass function in the Coma Berenices dwarf galaxy from deep near-infrared HST observations
• Signatures of Dark Matter Halo Expansion in Galaxy Populations
• Luminosity and Mass Function of the Galactic open cluster NGC 2422
• How radiation affects superbubbles: Through momentum injection in early phase and photo-heating thereafter
• Astrometric and photometric initial mass functions from the UKIDSS Galactic Clusters Survey: II The Alpha Persei open cluster
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• Deep Near-Infrared Imaging af an Embedded Cluster in the Extreme Outer Galaxy: Census of Supernovae Triggered Star Formation
• Nuclear embedded star clusters in NGC 7582
• The low mass star and sub-stellar populations of the 25 Orionis group
• The far-infrared - radio correlation in dwarf galaxies
• The origin of discrete multiple stellar populations in globular clusters
• The Elephant in the Room: The Importance of Where and When Massive Stars Form in Molecular Clouds
• Revisiting the classics: Is [Mg/Fe] a good proxy for galaxy formation time-scales?
• Compact Star Clusters in the M31 Disk
• The possible origin of the faint fuzzy star clusters in NGC 1023
• How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
• Encounters in the ONC - observing imprints of star-disc interactions
• Massive White Dwarfs in Young Star Clusters
• System IMF of the 25 Ori Group from Planetary-Mass Objects to Intermediate/High-Mass Stars
• Deep GeMS/GSAOI near-infrared observations of N159W in the Large Magellanic Cloud
• The central density of R136 in 30 Doradus
• Gradients of Stellar Population Properties and Evolution Clues in a Nearby Galaxy M 101
• EDGE: The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function
• Simulating a metallicity-dependent initial mass function: Consequences for feedback and chemical abundances
• The spatial and velocity distributions of hypervelocity stars
• Physical properties and chemical composition of the cores in the California molecular cloud
• Wolf-Rayet Galaxies in the Sloan Digital Sky Survey: the metallicity dependence of the initial mass function
• LMC self lensing for OGLE-II microlensing observations
• Chemical evolution of disc galaxies from cosmological simulations
• Optical and Near-infrared survey of the stellar contents associated with the star-forming Complex Sh2-252
• Cluster and nebular properties of the central star-forming region of NGC 1140
• Gravitational conundrum? Dynamical mass segregation versus disruption of binary stars in dense stellar systems
• Stellar cores in the Sh 2-305 H II region
• A Possible Solution for the M/L-[Fe/H] Relation of Globular Clusters in M31: A metallicity and density dependent top-heavy IMF
• Reading the CARDs: the Imprint of Accretion History in the Chemical Abundances of the Milky Way's Stellar Halo
• Strong dependence of the physical properties of cores on spatial resolution in observations and simulations
• Local stellar formation history from the 40 pc white dwarf sample
• Galactic Chemical Evolution and the Oxygen Isotopic Composition of the Solar System
• Boosting galactic outflows with enhanced resolution
• Probing the Upper Scorpius mass function in the planetary-mass regime
• A Wide Area Survey for High-redshift Massive Galaxies. II. Near-infrared Spectroscopy of BzK-selected Massive Star-forming Galaxies
• Radial Acceleration Relation between Baryons and Dark or Phantom Matter in the Super-critical Acceleration Regime of Nearly Spherical Galaxies
• [OIII] emission line as a tracer of star-forming galaxies at high redshifts: Comparison between H$\alpha$ and [OIII] emitters at $z$=2.23 in HiZELS
• Dissecting the Gaia HR diagram within 200 pc
• A joint analysis of the Drake equation and the Fermi paradox
• A Fresh Look at AGB stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass Relation
• Gamma rays from the Galactic bulge and large extra dimensions
• Low-mass young stellar population and star formation history of the cluster IC 1805 in the W4 H{\sc ii} region
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• A search for mass segregation of stars and brown dwarfs in ρ Ophiuchi
• The scale-free character of the cluster mass function and the universality of the stellar IMF
• Implications of a variable IMF for the interpretation of observations of galaxy populations
• How fast is mass-segregation happening in hierarchical formed embedded star clusters?
• Biases and systematics in the observational derivation of galaxy properties: comparing different techniques on synthetic observations of simulated galaxies
• Open cluster stability and the effects of binary stars
• Starburst-AGN mixing: TYPHOON observations of NGC 1365, NGC 1068, and the effect of spatial resolution on the AGN fraction
• Abundance determination of multiple star-forming regions in the HII galaxy SDSS J165712.75+321141.4
• The Star-forming Region NGC 346 in the Small Magellanic Cloud with Hubble Space Telescope ACS Observations. II. Photometric Study of the Intermediate-Age Star Cluster BS 90
• Binary Capture Rates for Massive Protostars
• The Quintuplet Cluster: Extended Structure and Tidal Radius
• Deep multi-telescope photometry of NGC 5466. I. Blue Stragglers and binary systems
• The initial mass function and star formation law in the outer disc of NGC 2915
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• Simulating the Legacy Survey of Space and Time stellar content with TRILEGAL
• The Binary Fraction and Mass Segregation in Alpha Persei Open Cluster
• Close Encounters of Stars with Stellar-mass Black Hole Binaries
• The SLUGGS survey: combining stars, globular clusters and planetary nebulae to understand the assembly history of early-type galaxies from their large radii kinematics
• Diffuse X-ray-emitting Gas in Major Mergers
• The first five years of gravitational-wave astrophysics
• Stellar populations across the black hole mass - velocity dispersion relation
• Star Formation in a Turbulent Framework: From Giant Molecular Clouds to Protostars
• A detailed study of the enigmatic cluster M82F
• SFR estimations from z=0 to z=0.9 -- A comparison of SFR calibrators for star-forming galaxies
• The Clustering Evolution of Dusty Star-Forming Galaxies
• On the inconsistency between cosmic stellar mass density and star formation rate up to $z\sim 8$
• Photometric and Kinematic study of the three intermediate age open clusters NGC 381, NGC 2360, and Berkeley 68
• The dynamical evolution of very-low mass binaries in open clusters
• Massive star formation in the GMC G345.5+1.0: Spatial distribution of the dust emission
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• Early-Forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
• Self-enrichment in globular clusters. I. An analytic approach
• Size distribution of superbubbles
• The Star Cluster System of the NGC 7673 Starburst
• Cradle(s) of the Sun
• Fragmentation in the Massive Star-Forming Region IRAS 19410+2336
• MiMO: Mixture Model for Open Clusters in Color-Magnitude Diagrams
• Predicting sub-millimeter flux densities from global galaxy properties
• Far and extreme ultraviolet radiation fields and consequent disc destruction in star-forming regions
• X-Ray Emission from Star-Forming Galaxies - Signatures of Cosmic Rays and Magnetic Fields
• Was the Milky Way a chain galaxy? Using the IGIMF theory to constrain the thin-disk star formation history and mass
• Comparing Models for IMF Variation Across Cosmological Time in Milky Way-like Galaxies
• Sejong Open Cluster Survey (SOS). III. The Young Open Cluster NGC 1893 in the H II Region W8
• Testing 24 micron and Infrared Luminosity as Star Formation Tracers for Galactic Star Forming Regions
• Sejong Open Cluster Survey (SOS). II. IC 1848 Cluster in the H II Region W5 West
• Does God play dice with star clusters?
• Crucial aspects of the initial mass function (I): The statistical correlation between the total mass of an ensemble of stars and its most massive star
• From the Outside Looking in: What can Milky Way Analogues Tell us About the Star Formation Rate of Our Own Galaxy?
• Why is the Milky Way X-factor Constant?
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• The Mass Function of omega Centauri down to 0.15 M_s
• A multi-wavelength census of stellar contents in the young cluster NGC 1624
• What does a universal IMF imply about star formation?
• Star Clusters in the Interacting Galaxy System Arp 284
• The last 5 Gyr of Galactic chemical evolution based on H II region abundances derived from a temperature independent method
• The History of Star Formation in Galaxy Disks in the Local Volume as Measured by the ACS Nearby Galaxy Survey Treasury
• The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
• Tracing star formation with non-thermal radio emission
• An All-Sky Sample of Intermediate-Mass Star-Forming Regions
• Protostar mass functions in young clusters
• An excessively massive thick disc of the enormous edge-on lenticular galaxy NGC7572
• High-resolution, 3D radiative transfer modelling V. A detailed model of the M51 interacting pair
• How do binary clusters form?
• The role of stellar expansion on the formation of gravitational wave sources
• Sixteen overlooked open clusters in the fourth Galactic quadrant. A combined analysis of UBVI photometry and Gaia DR2 with ASteCA
• NGC 7538 : Multiwavelength Study of Stellar Cluster Regions associated with IRS 1-3 and IRS 9 sources
• Auto-consistent metallicity and star formation history of the nearest blue compact dwarf galaxy NGC 6789
• New Insight into the stellar mass function of Galactic globular clusters
• Investigation of the stellar content in the western part of the Carina nebula
• The influence of a top-heavy integrated galactic IMF and dust on the chemical evolution of high-redshift starbursts
• Continuity of accretion from clumps to Class 0 high-mass protostars in SDC335
• The Lifetimes of Star Clusters Born with a Top-heavy IMF
• Creation/destruction of ultra-wide binaries in tidal streams
• Mass segregation in rich LMC clusters from modelling of deep HST colour-magnitude diagrams
• Extended Main Sequence Turn-Offs in Low Mass Intermediate Age Clusters
• A Mass-Dependent Yield Origin of Neutron-Capture Element Abundance Distributions in Ultra-Faint Dwarfs
• The Great Wave: Evidence of a large-scale vertical corrugation propagating outwards in the Galactic disc
• Cosmic evolution of metal densities: the enrichment of the Inter-Galactic Medium
• Optimal Integrated Abundances for Chemical Tagging of Extragalactic Globular Clusters
• The complex evolutionary paths of local infrared bright galaxies: a high angular resolution mid-infrared view
• Dark Matter Microhalos in the Solar Neighborhood: Pulsar Timing Signatures of Early Matter Domination
• Characterization of optically-selected star forming knots in (U)LIRGs
• Multi-wavelength study of a young open cluster NGC 7419
• The low-mass initial mass function of the field population in the Large Magellanic Cloud with Hubble Space Telescope WFPC2 Observations
• A Monte Carlo analysis of the velocity dispersion of the globular cluster Palomar 14
• Reading the tea leaves in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{sph}}$ and $M_{\mathrm{bh}}$-$R_{\mathrm{e},\mathrm{sph}}$ diagrams: dry and gaseous mergers with remnant angular momentum
• Did the Milky Way just light up? The recent star formation history of the Galactic disc
• HR-pyPopStar: high wavelength-resolution stellar populations evolutionary synthesis model
• On the Number of Stars in the Sun's Birth Cluster
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• Tightening the belt: Constraining the mass and evolution in SDC335
• Formation constraints indicate a black-hole accretor in 47 Tuc X9
• Origin of the dense core mass function in contracting filaments
• The origin of the LMC stellar bar: clues from the SFH of the bar and inner disk
• Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets
• Tests of star formation metrics in the low metallicity galaxy NGC 5253 using ALMA observations of H30$\alpha$ line emission
• Unveiling the physical conditions in NGC 6910
• Massive star cluster formation II. Runaway stars as fossils of sub-cluster mergers
• Rapid dynamical mass segregation and properties of fractal star clusters
• Characterizing Ultraviolet and Infrared Observational Properties for Galaxies. I. Influences of Dust Attenuation and Stellar Population Age
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• Photometric Properties of the Most Massive High-Redshift Galaxies
• Core dissolution and the dynamics of massive stars in young stellar clusters
• SN-driven mechanism of cusp-core transformation: an appraisal
• The slowest spinning X-ray pulsar in an extragalactic globular cluster
• Configurations of Bounded and Free-floating Planets in Very Young Open Clusters
• Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
• Raising the observed metallicity floor with a 3D non-LTE analysis of SDSS J102915.14+172927.9
• Measuring the Initial Mass Function of Low Mass Stars and Brown Dwarfs
• The complexity that the first stars brought to the Universe: Fragility of metal enriched gas in a radiation field
• Is the IMF in ellipticals bottom-heavy? Clues from their chemical abundances
• A photometric study of the Open Cluster II: Stellar population and dynamical evolution in NGC 559
• The initial conditions of isolated star formation - X. A suggested evolutionary diagram for prestellar cores
• The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
• Formation of massive binaries
• A WFI survey in the Chamaeleon II dark cloud
• The physics and modes of star cluster formation: simulations
• Model computations of blue stragglers and W UMa-type stars in globular clusters
• LBT and Spitzer Spectroscopy of Star-Forming Galaxies at 1 < z < 3: Extinction and Star Formation Rate Indicators
• No compelling evidence of significant early star cluster disruption in the Large Magellanic Cloud
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• Invoking the virial theorem to understand the impact of (dry) mergers on the $M_{\mathrm{bh}}$-$\sigma$ relation
• A Renaissance study of Am stars. I. The mass ratio distribution
• Exploring binary black hole mergers and host galaxies with Shark and COMPAS
• Disk fragmentation in high-mass star formation. High-resolution observations towards AFGL 2591-VLA 3
• Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution
• SNII enrichment and the star cluster mass function
• The Stellar Population And Origin Of The Mysterious High-Latitude Star Forming Cloud CG 12
• A Survey of Star Clusters in the M31 South-West Field. UBVRI Photometry and Multi-Band Maps
• The far-UV Interstellar Radiation Field in Galactic Disks: Numerical and Analytic Models
• Sejong Open Cluster Survey (SOS) - IV. The Young Open Clusters NGC 1624 and NGC 1931
• Testing the initial conditions and dynamical evolution of star clusters using Gaia - I
• The Initial Mass Function toward the low-mass end in the Large Magellanic Cloud with HST/WFPC2 Observations
• Young Brown Dwarfs in the Core of the W3 Main Star-Forming Region
• Elliptical galaxies kinematics within general relativity with renormalization group effects
• Mass distributions of stars and cores in young groups and clusters
• Infrared dark clouds on the far side of the Galaxy
• Momentum Injection by Clustered Supernovae: Testing Subgrid Feedback Prescriptions
• The mass function of IC4665 revisited by the UKIDSS Galactic Clusters Survey
• Constraining the Thin Disc Initial Mass Function using Galactic Classical Cepheids
• Close Encounters of Tight Binary Stars with Stellar-mass Black Holes
• The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
• Star-forming gas in young clusters
• Extranuclear Halpha-emitting complexes in low-z (U)LIRGs: Precursors of tidal dwarf galaxies?
• Mass function of a young cluster in a low-metallicity environment. Sh 2-209
• Characterizing Ultraviolet and Infrared Observational Properties for Galaxies. II. Features of Attenuation Law
• Physical properties, kinetics and mass function of 12 northern infrared dark clouds
• The galaxy-wide stellar initial mass function in the presence of cluster-to-cluster IMF variations
• On the evolution of intra-cluster gas within Galactic globular clusters
• Formation of proto-globular cluster candidates in cosmological simulations of dwarf galaxies at $z>4$
• The Nature of Parallax Microlensing Events Towards the Galactic Bulge
• The Circumgalactic Medium of Submillimeter Galaxies. I. First Results from a Radio-Identified Sample
• Discovery of $\sim$2200 new supernova remnants in 19 nearby star-forming galaxies with MUSE spectroscopy
• Outer regions of the merging system Arp 270
• Mass segregation in diverse environments
• The Probability Distribution of Astrophysical Gravitational-Wave Background Fluctuations
• The giants that were born swiftly -- Implications of the top-heavy stellar initial mass function on the birth conditions of globular clusters
• On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium
• Search for gas accretion imprints in voids: II. The galaxy Ark 18 as a result of a dwarf-dwarf merger
• The Young Stellar Population of the metal-poor galaxy NGC 6822
• Novel bounds on decaying axionlike particle dark matter from the cosmic background
• Planetary Nebula Candidates in Extragalactic Young Star Clusters
• Statistical stellar mass corrections for high-z galaxies observed with JWST broad-band filters due to template degeneracies
• An Analysis of the Population of Extended Main Sequence Turn-off Clusters in the Large Magellanic Cloud
• Stellar collisions in galactic centers: black hole growth and color gradients
• A multiwavelength investigation of the HII region S311: Young stellar population and star formation
• Parameter properties and stellar population of the old open cluster NGC 3960
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• PBH assisted search for QCD axion dark matter
• Dust attenuation in galaxies at cosmic dawn from the FirstLight simulations
• On the massive star content of the nearby dwarf irregular Wolf-Rayet galaxy IC 4662
• BATC 15 Band Photometry of the Open Cluster NGC 188
• Tentative Detection of the Circumgalactic Medium of the Isolated Low-Mass Dwarf Galaxy WLM
• The contribution of globular clusters to cosmic reionization
• Modeling Nearly Spherical Pure-bulge Galaxies with a Stellar Mass-to-Light Ratio Gradient under the $\Lambda$CDM and MOND Paradigms: I. Methodology, Dynamical Stellar Mass, and Fundamental Mass Plane
• On the evolutionary nature of puffed-up stripped star binaries and their occurrence in stellar populations
• Assessing the physical reality of Milky Way open cluster candidates
• Protostellar-disc fragmentation across all metallicities
• Splitting the lentils: Clues to galaxy/black hole coevolution from the discovery of offset relations for non-dusty versus dusty (wet-merger-built) lenticular galaxies in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ diagram
• Evaluating the Merger Rate of Binary Black Holes from Direct Captures and Third-Body Soft Interactions Using the Milky Way Globular Clusters
• A stellar population synthesis approach to the Oosterhoff dichotomy
• Near-infrared spectroscopy of the massive stellar population of W51: evidence for multi-seeded star formation
• S-Type and P-Type Habitability in Stellar Binary Systems: A Comprehensive Approach III. Results for Mars, Earth, and super-Earth Planets
• Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances
• Spectroscopic substellar initial mass function of NGC 2244
• The impact of episodic outflow feedback on stellar multiplicity and the star formation efficiency
• The Range of Variation of the Mass of the Most Massive Star in Stellar Clusters Derived from 35 Million Monte Carlo Simulations
• A comparison of the Milky Way's recent star formation revealed by dust thermal emission and high-mass stars
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• The SAMI Galaxy Survey: Gas Streaming and Dynamical M/L in Rotationally Supported Systems
• Study of Open Star Clusters Using the Gaia DR3: I- Poorly Studied King 2 and King 5
• Variation of the IMF
• Monte Carlo Simulations of Metal-Poor Star Clusters
• Low-mass pre--main-sequence stars in the Magellanic Clouds
• The Formation of Binary Star Clusters in the Milky Way and Large Magellanic Cloud
• Cosmic and Galactic Neutrino Backgrounds from Thermonuclear Sources
• Connecting Galactic and extragalactic outflows: From the Cygnus-X cluster to active galaxies
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• Extended star-forming region within galaxies in a dense proto-cluster core at z=2.53
• OGLE-2016-BLG-1266: A Probable Brown-Dwarf/Planet Binary at the Deuterium Fusion Limit
• Progenitor-mass-dependent yields amplify intrinsic scatter in dwarf-galaxy elemental abundance ratios
• Testing the star formation scaling relations in the clumps of the North American and Pelican cloud complexes
• Fifty Years of IMF Variation: The Intermediate-Mass Stars
• Chandra X-ray observation of the HII region Gum 31 in the Carina Nebula complex
• On the evolution of the observed Mass-to-Length relationship for star-forming filaments
• Kinematics of a globular cluster with an extended profile: NGC5694
• Discovery of a loose star cluster in the Large Magellanic Cloud
• The Massive M31 Cluster G1: Detailed Chemical Abundances from Integrated Light Spectroscopy
• The stellar content of the infalling molecular clump G286.21+0.17
• Massive Prestellar Cores in Radiation-magneto-turbulent Simulations of Molecular Clouds
• Near-infrared chemical abundances of stars in the Sculptor dwarf galaxy
• A discontinuity in the luminosity-mass relation and fluctuations in the evolutionary tracks of low-mass and low-metallicity stars at the Gaia M-dwarf gap
• Chandra X-ray observation of the young stellar cluster NGC 3293 in the Carina Nebula Complex
• Constraining neutrino-DM interactions with Milky Way dwarf spheroidals and supernova neutrinos
• AMICO-COSMOS galaxy cluster and group catalogue up to $z=2$: Sample properties and X-ray counterparts
• WIYN Open Cluster Study. XC. Radial-velocity Measurements and Spectroscopic Binary Orbits in the Open Cluster NGC 2506
• Low Mass Pre-Main Sequence stars in the Large Magellanic Cloud - II: HST-WFPC2 observations of two fields in the 30 Doradus region
• A Dual Power Law Distribution for the Stellar Initial Mass Function
• Drivers of disc tilting I: Correlations and possible drivers for Milky Way analogues
• pySTARBURST99: The Next Generation of STARBURST99
• Hydrodynamic simulations of the Disk of Gas Around Supermassive black holes (HDGAS) -I; Molecular Gas Dynamics
• An Early Catalog of Planet Hosting Multiple Star Systems of Order Three and Higher
• Understanding the Star Formation Efficiency in Dense Gas: Initial Results from the CAFFEINE Survey with ArTéMiS
• Photoevaporation of the Jovian circumplanetary disk I. Explaining the orbit of Callisto and the lack of outer regular satellites
• The initial mass function of stars and the star-formation rates of galaxies
• Stellar population synthesis models with a physically varying IMF
• Sh 2-301: a blistered H II region undergoing star formation
• Subarcsecond Imaging of the High-Mass Star Forming Region Onsala 1
• A deep study of an intermediate age open cluster SAI 35 (Juchert 20) using ground based imaging and Gaia EDR3 astrometry
• Evolution of star forming dwarf galaxies: Characterizing the star formation scenarios
• Stellar collisions in globular clusters: the origin of multiple stellar populations
• The star formation history of the LSB Galaxy UGC 5889
• Behind the Spotlight: A systematic assessment of outshining using NIRCam medium-bands in the JADES Origins Field
• G345.45+1.50: An expanding ring-like structure with massive star formation
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Mid Infrared View of the High Mass Star Formation Region W51A
• Investigating the Blue Straggler Stars radial distribution in globular clusters with Monte Carlo simulations
• Black Holes merging with Low Mass Gap Objects inside Globular Clusters
• Structural and Dynamical Analysis of the Quiescent Molecular Ridge in the Large Magellanic Cloud
• The formation of globular clusters with top-heavy initial mass functions
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
• Searching for Magnetar Binaries Disrupted by Core-Collapse Supernovae
• Investigating the ultraviolet and infrared radiation through the turbulent life of molecular clouds
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• The CMF as provenance of the stellar IMF ?
• An interferometric study of B star multiplicity
• Modeling IR Spectral Energy Distributions: A Pilot Study of Starburst Parameters and Silicate Absorption Curves for Some GOALS Galaxies
• The z = 9.625 Cosmic Gems Galaxy was a "Compact Blue Monster" Propelled by Massive Star Clusters
• A photoionization model of the spatial distribution of the optical and mid-IR properties in NGC595
• The Larson-Tinsley Effect in the UV: Interacting vs. `Normal' Spiral Galaxies
• Recent star formation episodes in the Galaxy: impact on its chemical properties and the evolution of its abundance gradient
• A modern view of galaxies and their stellar populations
• Analytic models of dust temperature in high-redshift galaxies
• The Distribution of UV Radiation Field in the Molecular Clouds of Gould Belt
• Stochastic processes, galactic star formation, and chemical evolution. Effects of accretion, stripping, and collisions in multiphase multi-zone models
• The study of two barred galaxies with curious kinematical features
• Large-scale environmental dependence of the abundance ratio of nitrogen to oxygen in blue, star-forming galaxies fainter than L*
• The Dependence of Prestellar Core Mass Distributions on the Structure of the Parental Cloud
• On the effects of rotation in primordial star-forming clouds
• Chemodynamical Properties and Ages of Metal-Poor Stars in S-PLUS
• Faint Stars in a Faint Galaxy: I. Ultra Deep Photometry of the Boötes I Ultra Faint Dwarf Galaxy
• Mapping the Spatial Distribution of Dust Extinction in NGC 959 Using Broadband Visible and mid-IR Filters
• Unbound stars hold the key to young star cluster history
• On the lifetime of discs around late type stars
• Simple stellar population models including blue stragglers
• Astrophysical properties of newly discovered Magellanic Cloud star clusters
• The VMC Survey - XXXII. Pre-main sequence populations in the Large Magellanic Cloud
• Spectral classification of young stars using conditional invertible neural networks I. Introducing and validating the method
• A deep wide-field optical survey in the young open cluster Collinder 359
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Stellar-wind feedback and magnetic fields around young compact star clusters: 3D MHD simulations
• The Equilibrium Tide: An Updated Prescription for Population Synthesis Codes
• Can star cluster environment affect dust input from massive AGB stars?
• Do fragmentation and accretion affect the stellar Initial Mass Function?
• A magnified view of star formation at redshift 0.9 from two lensed galaxies
• On the mass function of stars growing in a flocculent medium
• The MeerKAT Galaxy Clusters Legacy Survey: star formation in massive clusters at 0.15 < z < 0.35
• Accelerated structural evolution of galaxies in a starbursting cluster at z=2.51
• Massive young stellar objects in the Local Group spiral galaxy M33 identified using machine learning
• The Fornax3D project: Intrinsic Correlations between Orbital Properties and the Stellar Initial Mass Function
• Two-Point Separation Functions for Modeling Wide Binary Systems in Nearby Dwarf Galaxies
• The influence of the cloud virial parameter on the initial mass function
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• A Multiple Power Law Distribution for Initial Mass Functions
• Young stellar clumps in the interacting systems: Arp305
• Measuring Young Stars in Space and Time -- II. The Pre-Main-Sequence Stellar Content of N44
• Escaping stars from young low-N clusters
• H-ATLAS: The Far-Infrared properties of galaxies in and around the Coma Cluster
• A Near-Infrared Study of the Stellar Cluster: [DBS2003] 45
• Fragmentation and Evolution of Molecular Clouds. III: The Effect of Dust and Gas Energetics
• Influence of planets on debris disks in star clusters I: the 50 AU Jupiter
• Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data
• Astrometric mass measurement of compact companions in binary systems with Gaia
• First evidence of a stripped star cluster from the Small Magellanic Cloud
• COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction
• A spiral galaxy's mass distribution uncovered through lensing and dynamics
• Mass Modeling the Andromeda Dwarf Galaxies: Andromeda VI and Andromeda XXIII
• Simulations of Fractal Star Cluster Formation: I. New Insights for Measuring Mass Segregation of Star Clusters with SubStructure
• Hubble-Lemaître fragmentation and the path to equilibrium of merger-driven cluster formation
• A link between feedback outflows and satellite galaxy suppression
• Black hole mass function shift in proto-stellar-clusters driven by gas accretion
• Star Formation at the Galactic Center
• Stellar Populations in type Ia supernova host galaxies at intermediate-high redshift: Star formation and metallicity enrichment histories
• Making top-heavy IMFs from canonical IMFs near the Galactic Centre
• Massive stars in the young cluster VVV CL074
• Unveiling the Cosmic Gems Arc at $z\sim 10$ with JWST NIRCam
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Ionized Carbon in Galaxies: The [C II] 158 $\mu$m Line as a Total Molecular Gas Mass Tracer Revisited
• Star formation in the centre of NGC 1808 as observed by ALMA
• Multiwavelength study of the G345.5+1.5 region
• Giant molecular clouds and their Type classification in M74: Toward understanding star formation and cloud evolution
• Constraining the top-light initial mass function in the extended ultraviolet disk of M83
• The Physical Conditions in Starbursts Derived from Bayesian Fitting of Mid-IR SEDS: 30 Doradus as a Template
• Hypercompact stellar clusters: morphological renditions and spectro-photometric models
• Do Disk Galaxies with Abnormally Low Mass-to-Light Ratios Exist?
• Emergence of a stellar cusp by a dark matter cusp in a low-mass compact ultra-faint dwarf galaxy
• Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
• Crucial aspects of the initial mass function (II): The inference of total quantities from partial information on a cluster
• Fine structure in the luminosity function in young stellar populations with Gaia DR2
• On the Coagulation and Size Distribution of Pressure Confined Cores
• A Galactic Self-Portrait: Density Structure and Integrated Properties of the Milky Way Disk
• New method for estimating molecular cloud distances based on Gaia, 2MASS, and the TRILEGAL galaxy model
• Fitting Formulae and Constraints for the Existence of S-type and P-type Habitable Zones
• A new technique for the determination of the initial mass function in unresolved stellar populations
• On the IMF in a Triggered Star Formation Context
• The structure and early evolution of massive star forming regions - Substructure in the infrared dark cloud SDC13
• The impact of magnetic fields on the IMF in star-forming clouds near a supermassive black hole
• Theories of the initial mass function
• Bimodal Star Formation in Simulations of Strongly Magnetized Giant Molecular Clouds
• The Effect of Magnetic Fields and Ambipolar Diffusion on Core Mass Functions
• The Initial Mass Function as given by the fragmentation
• Explaining the stellar initial mass function with the theory of spatial networks
• Simulations of Dense Stellar Systems with the AMUSE Software Toolkit
• Galaxy Evolution in the Cluster Abell 85: New Insights from the Dwarf Population
• The Pristine survey: XXVII. The extremely metal-poor stream C-19 stretches over more than 100 degrees
• Impact of AGN and nuclear star formation on the ISM turbulence of galaxies: Insights from JWST/MIRI spectroscopy
• Monte-Carlo Modeling of Non-Gravitational Heating Processes in Galaxy Clusters
• The Dynamical Implications of Multiple Stellar Formation Events in Galactic Globular Clusters
• A young galaxy cluster in the old Universe
• Search for LBVs in the Local Volume galaxies: study of four stars in NGC 4449
• Very-wide-orbit planets from dynamical instabilities during the stellar birth cluster phase
• Spectroscopic Identification of Faint White Dwarf Candidates in the Praesepe Open Star Cluster
• Introducing a new multi-particle collision method for the evolution of dense stellar systems. Crash-test N-body simulations
• Dynamical mass of a star cluster in M83: a test of fibre-fed multi-object spectroscopy
• The Pristine Survey -- XXVII. Journey to the Galactic outskirts -- Mapping the outer halo red giant stars down to the very metal-poor end
• Evolution of thermal and nonthermal radio continuum emission on kpc scales--Predictions for SKA
• An HI shell-like structure associated with nova V458 Vulpeculae?
• Long-slit spectral observations and stellar mass-to-light ratio of spiral galaxy UGC11919
• Does slow and steady win the race? Investigating feedback processes in giant molecular clouds
• DECam Survey for Low-Mass Stars and Substellar Objects in the UCL and LCC Subgroups of the Sco-Cen OB Association (SCOCENSUS)
• Catching a Milky Way open cluster in its last breath
• Uncertainties in asteroseismic grid-based estimates of the ages of halo stars
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Kinematic scaling relations of disc galaxies from ionised gas at $z\sim 1$ and their connection with dark matter haloes
• Are hierarchically formed embedded star clusters surviving gas expulsion depending on their initial conditions?
• PAH Marks the Spot: Digging for Buried Clusters in Nearby Star-forming Galaxies
• Massive star cluster formation III. Early mass segregation during cluster assembly
• First Light And Reionisation Epoch Simulations (FLARES) XVI: Size Evolution of Massive Dusty Galaxies at Cosmic Dawn from UV to IR
• Frequency-Domain Distribution of Astrophysical Gravitational-Wave Backgrounds
• Formation of low-mass stars and brown dwarfs
• Comparing IMF-sensitive indices of intermediate-mass quiescent galaxies in various environments
• Deep V and I CCD photometry of young star cluster NGC 1893 with the 3.6m DOT
• Using microlensed quasars to probe the structure of the Milky Way
• Can Thorne-$\dot{\text{Z}}$ytkow Objects source GW190814-type events?
• New age-metallicity diagnostic diagram for the Washington photometric system
• The systematically varying stellar IMF
• WSRT observations and surface photometry of two unusual spiral galaxies
• Evolution of binaries with compact objects in globular clusters
• Generation of inclined protoplanetary discs and misaligned planets through mass accretion I: Coplanar secondary discs
• Star Formation in the Local Milky Way
• Gaia DR1 completeness within 250 pc and star formation history of the Solar neighbourhood
• Northern Galactic Molecular Cloud Clumps in Hi-GAL: Dense Gas Map and Environmental Trends
• Far-infrared - radio correlation and magnetic field strength in star-forming early-type galaxies
• Shocked POststarburst Galaxy Survey. IV. Outflows in Shocked Post-Starburst Galaxies Are Not Responsible For Quenching
• Globular cluster candidates in the Sagittarius dwarf galaxy
• Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation
• Stellar velocity distributions in binary-rich ultrafaint dwarf galaxies
• Fisher matrix forecasts on the astrophysics of galaxies during the epoch of reionisation from the 21-cm power spectra
• Dead Zones of Classical Habitability in Stellar Binary Systems
• Inferring the density and membership of stellar streams with flexible models: The GD-1 stream in Gaia Data Release 3
• GK Boo and AE For: Two low-mass eclipsing binaries with dwarf companions
• Complex stellar system ESO65SC03: Open cluster or remnant?
• Condition for low-mass star formation in shock-compressed metal-poor clouds
• The formation, disruption and properties of pressure-supported stellar systems and implications for the astrophysics of galaxies
• Short and long term evolution of a stellar disk around a massive black hole: The role of binaries, the cusp and stellar evolution
• Stellar Ages: A Code to Infer Properties of Stellar Populations
• The empirical upper limit for mass loss of cool main sequence stars
• Counting stars from the integrated spectra of galaxies
• Andromeda XXXV: The Faintest Dwarf Satellite of the Andromeda Galaxy
• Analysis of the Intrinsic Mid-Infrared L-band to Visible--Near-Infrared Flux Ratios in Spectral Synthesis Models of Composite Stellar Populations
• Molecular gas in cool-core brightest cluster galaxies at $z\simeq 0.4$
• Measuring Young Stars in Space and Time -- I. The Photometric Catalog and Extinction Properties of N44
• Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers
• Long-term investigation of an open cluster Berkeley 65
• Theoretical Color-Magnitude Diagrams and the Star Forming Histories of Interacting Open Multi-population Model Galaxies: Bursts and Busts
• Upper limit on the fraction of alien civilizations that develop communication technology
• Quantifying the Detectability of Milky Way Satellites with Image Simulations: a Case Study with KiDS
• Resonant Locking Between Binary Systems Induced by Gravitational Waves
• Photometric and Kinematic study of the open cluster NGC 1027
• Star clusters in the dwarf irregular galaxy Leo A
• Tidal effects on primordial black hole capture in neutron stars
• Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
• Supernova explosions of runaway stars and young neutron stars above the Galactic plane
• Cosmic-Ray Bath in a Past Supernova Gives Birth to Earth-Like Planets
• Simulations of the IMF in Clusters
• Using Source Proper Motion to Validate Terrestrial Parallax: OGLE-2019-BLG-1058
• Star-formation-rate estimates from water emission
• Massive binaries and the enrichment of the interstellar medium in globular clusters
• Aluminium-26 production in low- and intermediate-mass binary systems
• Understanding the IMF
• Observational properties of visual binaries as modelled using a synthetic catalogue, I: For visual apparent magnitudes $m_v<15$
• On the chemical evolution of the Milky Way
• Star Formation for Predictive Primordial Galaxy Formation
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Life Versus Dark Energy: How An Advanced Civilization Could Resist the Accelerating Expansion of the Universe
• Progenitor model of Cosmic Ray knee
• Searching for Low-mass Population III Stars Disguised as White Dwarfs
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Do Red Galaxies Form More Stars Than Blue Galaxies?
• A pilot method to determine the high mass end of the Stellar Initial Mass Function in galaxies using UVIT, H$\alpha$-MUSE observations and applied to NGC628
• The informativeness of [C II] line-intensity mapping as a probe of the H I content and metallicity of galaxies at the end of reionization
• When did the initial mass function become bottom-heavy?
• Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
• Early Stellar Flybys are Unlikely: Improved Constraints from Sednoids and Large-$q$ TNOs
• Light deflection in binary stars
• Dynamical Masses of Young Star Clusters: Constraints on the Stellar IMF and Star-Formation Efficiency
• Blue Stragglers in Clusters and Integrated Spectral Properties of Stellar Populations
• The evolution of the Oxygen abundance radial gradient in the Milky Way Galaxy disk
• Radio-to-Submillimetre Spectral Energy Distributions of NGC 1365
• Using the Modified Lognormal Power Law Distribution to Model the Mass Function of NGC 1711
• Tracing nitrogen enrichment across cosmic time with JWST
• Stability of a cluster-disrupted mean-motion resonance (chain) in HR 8799 and PDS 70
• Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33
• The large-scale kinematics of young stars in the Milky Way disc: first results from SDSS-V
• The ADF and the t${}^2$ formalism in H II regions based on the upper mass limit of the IMF for the MW
• MEGASTAR (III). Stellar parameters and data products for DR1 late-type stars
• Cosmic Radioactivity and Galactic Chemical Evolution
• The first stars
• Dynamical masses of early-type galaxies at z~2
• Centrally concentrated star formation in young clusters
• The Massive Star Forming Region, Cygnus OB2
• MASSCLEAN - MASSive CLuster Evolution and ANalysis Package - Description, Tests, and Results
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• Stochastic 2-D galaxy disk evolution models. Resolved stellar populations in the galaxy M33
• Oxford SWIFT IFS and multi-wavelength observations of the Eagle galaxy at z=0.77
• MeerKAT radio continuum imaging of nearby star-forming spirals in the NGC 6221, NGC 3256/3263, and NGC 2434 galaxy groups
• Local metallicity distribution function derived from Galactic large-scale radial iron pattern modelling
• Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
• The In Situ Growth of Stellar-mass "Light" Seed Black Holes in Nuclear Star Clusters
• A FUV-optical approach for studying hierarchical star formation in nearby galaxies with UVIT
• Semiresolved Stellar Populations as Distance Indicators
• The reason for the occurrence of W-type contact binaries
• Probing the farthest star clusters to the Small Magellanic Cloud
• Dips in the sub-TeV gamma-ray light curves from central parts of galaxies due to transiting luminous stars
• HR-pyPopStar II: high spectral resolution evolutionary synthesis models low metallicity expansion and the properties of the stellar populations of dwarf galaxies
• The mass-to-light ratio of rich star clusters
• X-ray emission of the Nuclear Stellar Disk as seen by SRG/ART-XC
• The sub-solar Initial Mass Function in the Large Magellanic Cloud
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• The Progenitor Systems of Classical Novae in M31
• Downsizing revised: Star formation timescales for elliptical galaxies with an environment-dependent IMF and number of SNIa
• Fornax 3D project: assessing the diversity of IMF and stellar population maps within the Fornax Cluster
• The interdependence between density PDF, CMF and IMF and their relation with Mach number in simulations
• Ultra-fast model emulation with PRISM; analyzing the Meraxes galaxy formation model
• Formation of Stellar Clusters and the Importance of Thermodynamics for Fragmentation
• Dynamical evolution of star clusters with top-heavy IMF
• An ancient system hidden in the Galactic plane?
• The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters
• The Future of IMF studies with the ELT and MICADO I: The local Universe as a resolved IMF laboratory
• Stars throw their weight in old galaxies
• Young Massive Clusters in Non-Interacting Galaxies
• Embedded Clusters and the IMF
• Estimating Galaxy Star Formation Rates from Murchison Widefield Array Radio Continuum Emission
• Neutron-capture elements record the ordered chemical evolution of the disc over time
• Revisiting a detached stellar structure in the outer northeastern region of the Small Magellanic Cloud
• Feedback and the Initial Mass function
• MASSIV: Mass Assembly Survey with SINFONI in VVDS. VI. Metallicity-related fundamental relations in star-forming galaxies at $1<z<2$
• Random fragmentation of turbulent molecular clouds lying in the central region of giant galaxies
• On the formation of massive stellar clusters
• Models of Late-Type Disk Galaxies: 1-D Versus 2-D
• Low-Mass Stars in the Sloan Digital Sky Survey: Galactic Structure, Kinematics, and the Luminosity Function
• SDSS-IV MaStar: Determination of Stellar Parameters Using Bayesian Averaging
• Survival of Protoplanetary Disks in Upper Scorpius from Population Synthesis Models with External Photoevaporation
• Star Formation Beyond the Optical Disk : The Low-Density Outskirts of NGC2090
• Gauging the Impact of Cosmic Ray Feedback on the Stellar Initial Mass Function