Zooming in on Individual Star Formation: Low- and High-mass Stars

Abstract

Star formation is a multi-scale, multi-physics problem ranging from the size scale of molecular clouds ($\sim$10s pc) down to the size scales of dense prestellar cores ($\sim$0.1 pc) that are the birth sites of stars. Several physical processes like turbulence, magnetic fields and stellar feedback, such as radiation pressure and outflows, are more or less important for different stellar masses and size scales. During the last decade a variety of technological and computing advances have transformed our understanding of star formation through the use of multi-wavelength observations, large scale observational surveys, and multi-physics multi-dimensional numerical simulations. Additionally, the use of synthetic observations of simulations have provided a useful tool to interpret observational data and evaluate the importance of various physical processes on different scales in star formation. Here, we review these recent advancements in both high- ($M\gtrsim 8M_{\odot }$) and low-mass star formation.

arXiv comment53 pages, 7 figures, To appear in Space Science Reviews (submitted January 31, 2020; accepted May 7, 2020), topical collection on Star formation

References in corpus (332)

• Galactic Stellar and Substellar Initial Mass Function
• The cosmological simulation code GADGET-2
• Star Formation in the Milky Way and Nearby Galaxies
• Theory of Star Formation
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Interstellar Dust Grains
• The Milky Way in Molecular Clouds: A New Complete CO Survey
• Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
• A Survey of Stellar Families: Multiplicity of Solar-Type Stars
• The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems
• Mass-loss predictions for O and B stars as a function of metallicity
• The Spitzer c2d Legacy Results: Star Formation Rates and Efficiencies; Evolution and Lifetimes
• From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey
• GIZMO: A New Class of Accurate, Mesh-Free Hydrodynamic Simulation Methods
• The Formation of Massive Stars from Turbulent Cores
• Cold Dark Clouds: The Initial Conditions for Star Formation
• Athena: A New Code for Astrophysical MHD
• Modelling Accretion in Protobinary Systems
• Complex Chemistry in Star-Forming Regions: An Expanded Gas-Grain Warm-up Chemical Model
• Interpreting Spectral Energy Distributions from Young Stellar Objects. I. A grid of 200,000 YSO model SEDs
• Characterizing interstellar filaments with Herschel in IC5146
• On the Star Formation Rates in Molecular Clouds
• Pulsational Pair-Instability Supernovae
• A Spitzer Survey of Young Stellar Clusters within One Kiloparsec of the Sun: Cluster Core Extraction and Basic Structural Analysis
• ATLASGAL - The APEX Telescope Large Area Survey of the Galaxy at 870 microns
• Gasoline: An adaptable implementation of TreeSPH
• Competitive accretion in embedded stellar cluster
• Herschel view of the Taurus B211/3 filament and striations: Evidence of filamentary growth?
• The Formation of Massive Star Systems by Accretion
• Gravitational Instabilities in Circumstellar Disks
• Stellar, brown dwarf and multiple star properties from a radiation hydrodynamical simulation of star cluster formation
• Wind-driven Accretion in Protoplanetary Disks. I: Suppression of the Magnetorotational Instability and Launching of the Magnetocentrifugal Wind
• Dynamics of Protoplanetary Disks
• High-Mass Star and Massive Cluster Formation in the Milky Way
• Filamentary structure of star-forming complexes
• The Star Formation Rate and Gas Surface Density Relation in the Milky Way: Implications for Extragalactic Studies
• The PLUTO Code for Adaptive Mesh Computations in Astrophysical Fluid Dynamics
• The mass function of dense molecular cores and the origin of the IMF
• Infrared Dark Clouds: precursors to star clusters
• The Spitzer Space Telescope Survey of the Orion A & B Molecular Clouds - Part I: A Census of Dusty Young Stellar Objects and a Study of their Mid-IR Variability
• On the formation of massive stars
• Probing the evolution of molecular cloud structure: From quiescence to birth
• Stellar, Brown Dwarf, and Multiple Star Properties from Hydrodynamical Simulations of Star Cluster Formation
• Properties of the Youngest Protostars in Perseus, Serpens, and Ophiuchus
• Efficiencies of Low-Mass Star and Star Cluster Formation
• Outflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster Forming Clumps
• Global collapse of molecular clouds as a formation mechanism for the most massive stars
• The Physics of Star Formation
• Global Hierarchical Collapse In Molecular Clouds. Towards a Comprehensive Scenario
• ATLASGAL --- properties of a complete sample of Galactic clumps
• Cluster-formation in the Rosette molecular cloud at the junctions of filaments
• Bolocam Survey for 1.1 mm Dust Continuum Emission in the c2d Legacy Clouds. I. Perseus
• Gas and grain chemical composition in cold cores as predicted by the Nautilus 3-phase model
• Filamentary Accretion Flows in the Embedded Serpens South Protocluster
• Simulating Radiating and Magnetized Flows in Multi-Dimensions with ZEUS-MP
• The Effects of Radiative Transfer on Low-Mass Star Formation
• The Evolution of Outflow-Envelope Interactions in Low-Mass Protostars
• Protostellar disk formation and transport of angular momentum during magnetized core collapse
• Young Stellar Objects in the Gould Belt
• Low Virial Parameters in Molecular Clouds: Implications for High Mass Star Formation and Magnetic Fields
• Global simulations of protoplanetary disks with ohmic resistivity and ambipolar diffusion
• The Taurus Spitzer Survey: New Candidate Taurus Members Selected Using Sensitive Mid-Infrared Photometry
• The Importance of Radiative Feedback for the Stellar Initial Mass Function
• The Formation of Low-Mass Binary Star Systems Via Turbulent Fragmentation
• Embedding Lagrangian Sink Particles in Eulerian Grids
• An excess of massive stars in the local 30 Doradus starburst
• Water in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results
• Bolocam Survey for 1.1 mm Dust Continuum Emission in the c2d Legacy Clouds. II. Ophiuchus
• Inefficient star formation through turbulence, magnetic fields and feedback
• Protostellar Turbulence Driven by Collimated Outflows
• Gravity or Turbulence? The velocity dispersion-size relation
• Evolution of Massive Protostars via Disk Accretion
• The impact of magnetic fields on single and binary star formation
• KROME - a package to embed chemistry in astrophysical simulations
• A Triple Protostar System Formed via Fragmentation of a Gravitationally Unstable Disk
• TADPOL: A 1.3 mm Survey of Dust Polarization in Star-forming Cores and Regions
• LIME - a flexible, non-LTE line excitation and radiation transfer method for millimeter and far-infrared wavelengths
• SDC13 infrared dark clouds: Longitudinally collapsing filaments?
• On Why Disks Generate Magnetic Towers and Collimate Jets
• H II regions: Witnesses to massive star formation
• An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud
• Disk-mediated accretion burst in a high-mass young stellar object
• A Correlation Between Surface Densities of Young Stellar Objects and Gas in Eight Nearby Molecular Clouds
• HYPERION: An open-source parallelized three-dimensional dust continuum radiative transfer code
• Radiation Magnetohydrodynamic Simulations of Protostellar Collapse: Protostellar Core Formation
• Collapse of massive magnetized dense cores using radiation-magneto-hydrodynamics: early fragmentation inhibition
• The Interplay of Magnetic Fields, Fragmentation and Ionization Feedback in High-Mass Star Formation
• Disk formation during collapse of magnetized protostellar cores
• An Ammonia Spectral Atlas of Dense Cores in Perseus
• Fragmentation at the Earliest Phase of Massive Star Formation
• Characterizing the properties of nearby molecular filaments observed with Herschel
• Direct observation of a sharp transition to coherence in Dense Cores
• The ALMA Survey of 70 $\mu$m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation
• Resolving the Luminosity Problem in Low-Mass Star Formation
• Dense core formation by fragmentation of velocity-coherent filaments in L1517
• A Classification Scheme for Young Stellar Objects Using the WIDE-FIELD INFRARED SURVEY EXPLORER AllWISE Catalog: Revealing Low-Density Star Formation in the Outer Galaxy
• The dusty MOCASSIN: fully self-consistent 3D photoionisation and dust radiative transfer models
• Radiation-Hydrodynamic Simulations of the Formation of Orion-Like Star Clusters II. The Initial Mass Function from Winds, Turbulence, and Radiation
• Collapse, outflows and fragmentation of massive, turbulent and magnetized prestellar barotropic cores
• The thermodynamics of collapsing molecular cloud cores using smoothed particle hydrodynamics with radiative transfer
• Fragmentation of Molecular Clumps and Formation of Protocluster
• Radiation Magnetohydrodynamic Simulations of Protostellar Collapse: Non-Ideal Magnetohydrodynamic Effects and Early Formation of Circumstellar Disks
• A "Starless" Core that Isn't: Detection of a Source in the L1014 Dense Core with the Spitzer Space Telescope
• A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey
• The Fragmentation of Magnetized, Massive Star-Forming Cores with Radiative Feedback
• On the nature of star-forming filaments: I. Filament morphologies
• A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency. First Tests
• Radiative transfer with POLARIS: I. Analysis of magnetic fields through synthetic dust continuum polarization measurements
• A Herschel and APEX Census of the Reddest Sources in Orion: Searching for the Youngest Protostars
• The James Clerk Maxwell Telescope Legacy Survey of Nearby Star-forming Regions in the Gould Belt
• The Circumstellar Environment of High Mass Protostellar Objects. III Evidence of Infall?
• The earliest phases of star formation - A Herschel key project. The thermal structure of low-mass molecular cloud cores
• Astrochemistry of dust, ice and gas: introduction and overview
• Misalignment of Magnetic Fields and Outflows in Protostellar Cores
• Formation Process of the Circumstellar Disk: Long-term Simulations in the Main Accretion Phase of Star Formation
• Effect of Magnetic Braking on the Circumstellar Disk Formation in a Strongly Magnetized Cloud
• SMA Observations of Class 0 Protostars: A High-Angular Resolution Survey of Protostellar Binary Systems
• The Spitzer c2d Survey of Nearby Dense Cores: II: Discovery of a Low Luminosity Object in the "Evolved Starless Core" L1521F
• The COMPLETE Survey of Outflows in Perseus
• Radiative transfer and the energy equation in SPH simulations of star formation
• The Green Bank Ammonia Survey (GAS): First Results of NH3 mapping the Gould Belt
• Can non-ideal magnetohydrodynamics solve the magnetic braking catastrophe?
• A test suite for quantitative comparison of hydrodynamics codes in astrophysics
• Protostellar collapse: radiative and magnetic feedbacks on small scale fragmentation
• Radiation hydrodynamics with Adaptive Mesh Refinement and application to prestellar core collapse. I Methods
• Dynamics of Dense Cores in the Perseus Molecular Cloud
• The JCMT Gould Belt Survey: First results from the SCUBA-2 observations of the Ophiuchus molecular cloud and a virial analysis of its prestellar core population
• Turbulent Molecular Cloud Cores: Rotational Properties
• A distance limited sample of massive molecular outflows
• Protostellar Disk Formation Enabled by Removal of Small Dust Grains
• Collapse of a molecular cloud core to stellar densities: stellar core and outflow formation in radiation magnetohydrodynamics simulations
• Magnetic fields during the early stages of massive star formation - I. Accretion and disk evolution
• On the nature of star-forming filaments: II. Sub-filaments and velocities
• The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament
• Protostars: Forges of cosmic rays?
• Current Star Formation in the Ophiuchus and Perseus Molecular Clouds: Constraints and Comparisons from Unbiased Submillimeter and Mid-Infrared Surveys. II
• UCLCHEM: A Gas-Grain Chemical Code
• Effects of Ohmic and ambipolar diffusion on the formation and evolution of the first cores, protostars and circumstellar discs
• A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey
• Conditions for Circumstellar Disk Formation: Effects of Initial Conditions and Sink Treatment
• Radiation-Hydrodynamic Simulations of Massive Star Formation with Protostellar Outflows
• Evolution of Protostellar Outflow around Low-mass Protostar
• Molecular Outflows Driven by Low-Mass Protostars. I. Correcting for Underestimates When Measuring Outflow Masses and Dynamical Properties
• The Link between Magnetic Fields and Filamentary Clouds: Bimodal Cloud Orientations in the Gould Belt
• Current Star Formation in the Perseus Molecular Cloud: Constraints from Unbiased Submillimeter and Mid-Infrared Surveys
• Molecular Line Emission as a Tool for Galaxy Observations (LEGO). I. HCN as a tracer of moderate gas densities in molecular clouds and galaxies
• Understanding Spatial and Spectral Morphologies of Ultracompact H II Regions
• Inefficient star formation: The combined effects of magnetic fields and radiative feedback
• An Unstable Truth: How Massive Stars get their Mass
• The influence of turbulence during magnetized core collapse and its consequences on low-mass star formation
• Molecular clouds have power-law probability distribution functions
• Evolution of column density distributions within Orion~A
• Magnetically regulated collapse in the B335 protostar ? I. ALMA observations of the polarized dust emission
• Turbulence-induced disc formation in strongly magnetised cloud cores
• The Star Formation Rate in the Gravoturbulent Interstellar Medium
• Embedded Protostars in the Dust, Ice, and Gas In Time (DIGIT) Key Program: Continuum SEDs, and an Inventory of Characteristic Far-Infrared Lines from PACS Spectroscopy
• A candidate circumbinary Keplerian disk in G35.20-0.74 N: A study with ALMA
• A submillimetre survey of the kinematics of the Perseus molecular cloud - II. Molecular outflows
• First hydrodynamics simulations of radiation forces and photoionization feedback in massive star formation
• The Turbulent Origin of Spin-Orbit Misalignment in Planetary Systems
• Herschel observations of B1-bS and B1-bN: two first hydrostatic core candidates in the Perseus star-forming cloud
• A recent accretion burst in the low-mass protostar IRAS 15398-3359: ALMA imaging of its related chemistry
• Close companions around young stars
• 3D-PDR: A new three-dimensional astrochemistry code for treating Photodissociation Regions
• CARMA observations of protostellar outflows in NGC 1333
• The early stages of star formation in Infrared Dark Clouds: characterizing the core dust properties
• Gravity drives the evolution of infrared dark hubs: JVLA observations of SDC13
• Class 0 Protostars in the Perseus Molecular Cloud: A Correlation Between the Youngest Protostars and the Dense Gas Distribution
• Dynamics of cluster-forming hub-filament systems: The case of the high-mass star-forming complex Monoceros R2
• Fast and accurate frequency-dependent radiation transport for hydrodynamics simulations in massive star formation
• Filamentary Fragmentation and Accretion in High-Mass Star-Forming Molecular Clouds
• Gravity or turbulence? -III. Evidence of pure thermal Jeans fragmentation at ~0.1 pc scale
• Balloon-Borne Submillimeter Polarimetry of the Vela C Molecular Cloud: Systematic Dependence of Polarization Fraction on Column Density and Local Polarization-Angle Dispersion
• CARMA Large Area Star Formation Survey: Observational Analysis of Filaments in the Serpens South Molecular Cloud
• Quantifying Observational Projection Effects Using Molecular Cloud Simulations
• Two Mass Distributions in the L 1641 Molecular Clouds: The Herschel connection of Dense Cores and Filaments in Orion A
• Interferometric observations of magnetic fields in forming stars
• The Mass Distributions of Starless and Protostellar Cores in Gould Belt Clouds
• Schmidt's Conjecture and Star Formation in Molecular Clouds
• The Earliest Phases of Star formation observed with Herschel (EPoS): The dust temperature and density distributions of B68
• HAWC+/SOFIA Multiwavelength Polarimetric Observations of OMC-1
• ALMA observations of dust polarization and molecular line emission from the Class 0 protostellar source Serpens SMM1
• Protostellar birth with ambipolar and ohmic diffusion
• Gone With the Wind: Where is the Missing Stellar Wind Energy from Massive Star Clusters?
• Radiation Magnetohydrodynamics Simulation of Proto-Stellar Collapse: Two-Component Molecular Outflow
• HOPS 383: An Outbursting Class 0 Protostar in Orion
• Collapse of a molecular cloud core to stellar densities: the formation and evolution of pre-stellar discs
• Simulating the Formation of Massive Protostars: I. Radiative Feedback and Accretion Disks
• Impact of Protostellar Outflows on Turbulence and Star Formation Efficiency in Magnetized Dense Cores
• Probing the evolution of molecular cloud structure II: From chaos to confinement
• Feedback Effects on Low-Mass Star Formation
• The earliest phases of high-mass star formation, as seen in NGC 6334 by \emph{Herschel}
• A necklace of dense cores in the high-mass star forming region G35.20-0.74N: ALMA observations
• Investigations of Protostellar Outflow Launching and Gas Entrainment: Hydrodynamic Simulations and Molecular Emission
• Importance of the Initial Conditions for Star Formation - III: Statistical Properties of Embedded Protostellar Clusters
• L1448 IRS2E: A candidate first hydrostatic core
• A closer look at the "characteristic" width of molecular cloud filaments
• Gas flow and accretion via spiral streamers and circumstellar disks in a young binary protostar
• Magnetized Interstellar Molecular Clouds. I. Comparison Between Simulations and Zeeman Observations
• Infall Signatures in a Prestellar Core embedded in the High-Mass 70 $\mu$m Dark IRDC G331.372-00.116
• Molecular Line Emission from Massive Protostellar Disks: Predictions for ALMA and the EVLA
• The role of magnetic fields in the formation of protostellar discs
• ALMA survey of massive cluster progenitors from ATLASGAL. Limited fragmentation at the early evolutionary stage of massive clumps
• Testing Larson's relationships in massive clumps
• Detection of Infall in the Protostar B335 with ALMA
• Submillimeter and Far-Infrared Polarimetric Observations of Magnetic Fields in Star-Forming Regions
• Simulations of protostellar collapse using multigroup radiation hydrodynamics. II. The second collapse
• The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Perseus Protostars. VI. Characterizing the Formation Mechanism for Close Multiple Systems
• A Keplerian disk around Orion Source I, a ~15 Msun YSO
• The Green Bank Ammonia Survey: Dense Cores Under Pressure in Orion A
• Outflow-Confined H II Regions. I. First Signposts of Massive Star Formation
• Protostellar Outflows and Radiative Feedback from Massive Stars. II. Feedback, Star Formation Efficiency, and Outflow Broadening
• A holistic perspective on the dynamics of G035.39-00.33: the interplay between gas and magnetic fields
• On the reliability of protostellar disc mass measurements and the existence of fragmenting discs
• Stellar feedback as the origin of an extended molecular outflow in a starburst galaxy
• The shapes of column density PDFs - The importance of the last closed contour
• Dust Polarization Toward Embedded Protostars in Ophiuchus with ALMA. I. VLA 1623
• The Effects of Magnetic Fields and Protostellar Feedback on Low-mass Cluster Formation
• On the stability of radiation-pressure-dominated cavities
• Formation and Evolution of Disks around Young Stellar Objects
• The Formation and Evolution of Wide-Orbit Stellar Multiples In Magnetized Clouds
• Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons
• The role of molecular filaments in the origin of the prestellar core mass function and stellar initial mass function
• Protostellar Disk Formation Enabled by Weak, Misaligned Magnetic Fields
• Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurements
• Resolving the polarized dust emission of the disk around the massive star powering the HH~80-81 radio jet
• A First Look at BISTRO Observations of The $\rho$ Oph-A core
• The Pillars of Creation revisited with MUSE: gas kinematics and high-mass stellar feedback traced by optical spectroscopy
• Droplets I: Pressure-Dominated Sub-0.1 pc Coherent Structures in L1688 and B18
• The collapse of a molecular cloud core to stellar densities using radiation non-ideal magnetohydrodynamics
• Massive Outflows Driven by Magnetic Effects in Star Forming Clouds with High Mass Accretion Rates
• Hierarchical fragmentation in the Perseus molecular cloud: From the cloud scale to protostellar objects
• The Necessity of Feedback Physics in Setting the Peak of the Initial Mass Function
• The disk-outflow system in the S255IR area of high mass star formation
• HiRes Deconvolved Spitzer Images of 89 Protostellar Jets and Outflows: New Data on Evolution of Outflow Morphology
• An ALMA Search for Substructure, Fragmentation, and Hidden Protostars in Starless Cores in Chamaeleon I
• JCMT BISTRO Survey observations of the Ophiuchus Molecular Cloud: Dust grain alignment properties inferred using a Ricean noise model
• Exploration of Cosmic Ray Acceleration in Protostellar Accretion Shocks and A Model for Ionization Rates in Embedded Protoclusters
• The First Two Thousand Years of Star Formation
• Observing Simulated Protostars with Outflows: How Accurate are Protostellar Properties Inferred from SEDs?
• Massive outflows associated with ATLASGAL clumps
• Jets and outflows of massive protostars - From cloud collapse to jet launching and cloud dispersal
• A $Herschel-SPIRE$ Survey of the Mon R2 Giant Molecular Cloud: Analysis of the Gas Column Density Probability Density Function
• VLA and CARMA Observations of Protostars in the Cepheus Clouds: Sub-arcsecond Proto-Binaries Formed via Disk Fragmentation
• A Stable, Accurate Methodology for High Mach Number, Strong Magnetic Field MHD Turbulence with Adaptive Mesh Refinement: Resolution and Refinement Studies
• The role of cosmic rays on magnetic field diffusion and the formation of protostellar discs
• A catalogue of dense cores and young stellar objects in the Lupus complex based on Herschel Gould Belt Survey observations
• The dense cores and filamentary structure of the molecular cloud in Corona Australis. Herschel SPIRE and PACS observations from the Herschel Gould Belt Survey
• Near-Infrared High-Resolution Imaging Polarimetry of FU Ori-Type Objects: Towards A Unified Scheme for Low-Mass Protostellar Evolution
• The Onset of Massive Star Formation: The Evolution of Temperature and Density Structure in an Infrared Dark Cloud
• An Ammonia Spectral Map of the L1495-B218 Filaments in the Taurus Molecular Cloud : I. Physical Properties of Filaments and Dense cores
• Effect of Angular Momentum Alignment and Strong Magnetic Fields on the Formation of Protostellar Disks
• Magnetic field morphology in nearby molecular clouds as revealed by starlight and submillimetre polarization
• Gravity or turbulence? IV. Collapsing cores in out-of-virial disguise
• The Anatomy of the Column Density Probability Distribution Function (N-PDF)
• Dust Polarization Toward Embedded Protostars in Ophiuchus with ALMA. II. IRAS 16293-2422
• Massive and low-mass protostars in massive "starless" cores
• The search for high-mass protostars with ALMA revealed up to kilo-parsec scales (SPARKS): I. Indication for a centrifugal barrier in the environment of a single high-mass envelope
• A Hot and Massive Accretion Disk around the High-Mass Protostar IRAS 20126+4104
• Stellar clusterings around "Isolated" Massive YSOs in the LMC
• The Kinematics of Molecular Cloud Cores in the Presence of Driven and Decaying Turbulence: Comparisons with Observations
• What Physics Determines the Peak of the IMF? Insights from the Structure of Cores in Radiation-Magnetohydrodynamic Simulations
• Herschel Observations of a Potential Core Forming Clump: Perseus B1-E
• Mass Assembly of Stellar Systems and Their Evolution with the SMA (MASSES). Multiplicity and the Physical Environment in L1448N
• Radiative Rayleigh-Taylor instabilities
• What Sets the Initial Rotation Rates of Massive Stars?
• Simulations of protostellar collapse using multigroup radiation hydrodynamics. I. The first collapse
• The Astrochemical Impact of Cosmic Rays in Protoclusters I: Molecular Cloud Chemistry
• The effect of magnetic fields on the formation of circumstellar discs around young stars
• ALMA Observations of Starless Core Substructure in Ophiuchus
• The far-infrared polarization spectrum of Rho Ophiuchi A from HAWC+/SOFIA observations
• The effect of episodic accretion on the phase transition of CO and CO_2 in low-mass star formation
• Fragmenting protostellar disks: properties and observational signatures
• ALMA observations of a misaligned binary protoplanetary disk system in Orion
• Massive Star Formation via the Collapse of Subvirial and Virialized Turbulent Massive Cores
• Radiation-hydrodynamical simulations of massive star formation using Monte Carlo radiative transfer II. The formation of a 25 solar-mass star
• The FRIGG project: From intermediate galactic scales to self-gravitating cores
• Embedded Binaries and Their Dense Cores
• Hybrid Adaptive Ray-Moment Method (HARM${}^2$): A Highly Parallel Method for Radiation Hydrodynamics on Adaptive Grids
• A grid of 1D low-mass star formation collapse models
• ALMA Observations of Orion Source I at 350 and 660 GHz
• TORUS-3DPDR: A self-consistent code treating three-dimensional photoionization and photodissociation regions
• When H II Regions are Complicated: Considering Perturbations from Winds, Radiation Pressure, and Other Effects
• An Asymmetric Keplerian Disk Surrounding the O-type Protostar IRAS16547$-$4247
• Synthetic Observations of Magnetic Fields in Protostellar Cores
• Synthetic observations of star formation and the interstellar medium
• First Core Properties: From Low- to High-mass Star Formation
• Mass Assembly of Stellar Systems and their Evolution with the SMA - 1.3 mm Subcompact Data Release
• The RMS Survey: Ammonia mapping of the environment of massive young stellar objects
• ALMA reveals a candidate hot and compact disk around the O-type protostar IRAS 16547$-$4247
• On the effects of optically thick gas (disks) around massive stars
• Simulations of star formation in Ophiuchus, II: Multiplicity
• Magnetically-regulated fragmentation of a massive, dense and turbulent clump
• Bondi-Hoyle Accretion in an Isothermal Magnetized Plasma
• Multi-scale dynamics in star-forming regions: the interplay between gravity and turbulence
• High-mass star formation at sub-50AU scales
• Initial Fragmentation in the Infrared Dark Cloud G28.53-0.25
• Geometry, Kinematics, and Magnetization of Simulated Prestellar Cores
• Asymmetric Line Profiles in Dense Molecular Clumps Observed in MALT90: Evidence for Global Collapse
• Herschel far-infrared photometric monitoring of protostars in the Orion Nebula Cluster
• The Mass Evolution of Protostellar Disks and Envelopes in the Perseus Molecular Cloud
• Hall effect-driven formation of gravitationally unstable discs in magnetized molecular cloud cores
• The effect of extreme ionisation rates during the initial collapse of a molecular cloud core
• Zooming in to Massive Star Birth
• The fragmentation properties of massive protocluster gas clumps: an ALMA study
• A new hybrid radiative transfer method for massive star formation
• Populations of Young Stellar Objects in Nearby Molecular Clouds
• The JCMT Transient Survey: Identifying Submillimetre Continuum Variability over Several Year Timescales Using Archival JCMT Gould Belt Survey Observations
• CASI: A Convolutional Neural Network Approach for Shell Identification
• Evidence for disks at an early stage in class 0 protostars?
• Early science with the Large Millimetre Telescope: An LMT/AzTEC 1.1 mm Survey of Dense Cores in the Monoceros R2 Giant Molecular Cloud
• Mapping the core mass function onto the stellar IMF: multiplicity matters
• Spectroscopic Analysis of an EIT Wave/Dimming Observed by Hinode/EIS
• An Ammonia Spectral Map of the L1495-B218 Filaments in the Taurus Molecular Cloud: II CCS & HC${}_7$N Chemistry and Three Modes of Star Formation in the Filaments
• Results from HOPS: A Multiwavelength Census of Orion Protostars
• Lack of high-mass prestellar cores in the starless MDCs of NGC6334
• Widening of Protostellar Outflows: an Infrared Outflow Survey in Low Luminosity Objects
• The circumestellar disk of the B0 protostar powering the HH 80-81 radio jet
• Investigating the Complex Velocity Structures within Dense Molecular Cloud Cores with GBT-Argus
• Synthetic Observations of the Evolution of Starless Cores in a Molecular Cloud Simulation: Comparisons with JCMT Data and Predictions for ALMA
• Impact of Cosmic-Ray Feedback on Accretion and Chemistry in Circumstellar Disks
• Fragmentation, rotation and outflows in the high-mass star-forming region IRAS 23033+5951. A case study of the IRAM NOEMA large program CORE
• On the relative motions of dense cores and envelopes in star-forming molecular clouds
• The structure of molecular gas associated with NGC2264: wide-field 12CO and H2 imaging
• Line-driven ablation of circumstellar discs: IV. The role of disc ablation in massive star formation and its contribution to the stellar upper mass limit
• Assessing the Performance of a Machine Learning Algorithm in Identifying Bubbles in Dust Emission
• A turbulent origin for the complex envelope kinematics in the young low-mass core Per-Bolo 58
• The Envelope Kinematics and a Possible Disk Around the Class 0 Protostar within BHR7
• Effects of infall and outflow on massive star-forming regions
• Gravitational instabilities in a protosolar-like disc III: molecular line detection and sensitivities
• Predictions for Observing Protostellar Outflows with ALMA
• The Disappearing Envelope around the Transitional Class I Object L43

Cited by in corpus (34)

• Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
• Multi-directional mass-accretion and collimated outflows in W51
• Evolution of Stellar Feedback in HII Regions
• The Role of Outflows, Radiation Pressure, and Magnetic Fields in Massive Star Formation
• Comparing the pre-SNe feedback and environmental pressures for 6000 HII regions across 19 nearby spiral galaxies
• Turbulence, Coherence and Collapse: Three Phases for Core Evolution
• Formation and evolution of a protoplanetary disk: combining observations, simulations and cosmochemical constraints
• A Massive Star is Born: How Feedback from Stellar Winds, Radiation Pressure, and Collimated Outflows Limits Accretion onto Massive Stars
• PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
• The Effects of Magnetic Fields and Outflow Feedback on the Shape and Evolution of the Density PDF in Turbulent Star-Forming Clouds
• VETTAM: A scheme for radiation hydrodynamics with adaptive mesh refinement using the variable Eddington tensor method
• Continuity of accretion from clumps to Class 0 high-mass protostars in SDC335
• Physical and chemical complexity in high-mass star-forming regions with ALMA. I. Overview and evolutionary trends of physical properties
• HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules -- I. Survey description and a first look toward W3(OH), W3 IRS5 and NGC 7538 IRS1
• JOYS: Disentangling the warm and cold material in the high-mass IRAS 23385+6053 cluster
• Clustered star formation at early evolutionary stages. Physical and chemical analysis of the young star-forming regions ISOSS J22478+6357 and ISOSS J23053+5953
• Unraveling the observational signatures of cloud-cloud collision and hub-filament systems in W31
• The SEDIGISM survey: Molecular cloud morphology. I. Classification and star formation
• Comparing Be Star Inclination Angles Determined from H$\alpha$ Fitting and Gravitational Darkening
• AFGL 5180 and AFGL 6366S: sites of hub-filament systems at the opposite edges of a filamentary cloud
• The disk-outflow system around the rare young O-type protostar W42-MME
• Unraveling the inner substructure of new candidate hub-filament system in the HII region G25.4NW
• A spectral survey of CH3CCH in the Hot Molecular Core G331.512-0.103
• The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"
• Fine structure and kinematics of the ionized and molecular gas in the jet and disk around S255IR NIRS3 from high resolution ALMA observations
• Massive extended streamers feed high-mass young stars
• A High Angular Resolution Survey of Massive Stars in Cygnus OB2: $JHK$ Adaptive Optics Results from the Gemini Near-InfraRed Imager
• Study of the high-mass star-forming region S255IR at various scales
• Ionized filaments and ongoing physical processes in massive star-forming sites around l = 345.5 degree
• ALMA discovery of a dual dense probably rotating outflow from a massive young stellar object G18.88MME
• APEX survey of interstellar HCl: ${}^{35}$Cl/${}^{37}$Cl isotopic ratios in dense cores and outflows
• Linking simulations and observations of star-forming regions I. Masses and temperatures of ALMAGAL-like cores
• Setting the Stage: The Early History of the Solar System
• Discs and outflows in the early phases of massive star formation: influence of magnetic fields and ambipolar diffusion