Ralf Klessen
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German astronomer
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(Suggest an Edit or Addition)According to Wikipedia, Ralf Stephan Klessen is a German astronomer. He is a professor of theoretical astrophysics at the Institute of Theoretical Astrophysics, part of the Center for Astronomy at the University of Heidelberg, Germany, and is currently the Managing Director of the Institute, as well as a Deputy Director of the Center for Astronomy.
Ralf Klessen's Published Works
Published Works
- Control of star formation by supersonic turbulence (2000) (1223)
- Comparing the statistics of interstellar turbulence in simulations and observations - Solenoidal versus compressive turbulence forcing (2009) (579)
- THE STAR FORMATION RATE OF TURBULENT MAGNETIZED CLOUDS: COMPARING THEORY, SIMULATIONS, AND OBSERVATIONS (2012) (432)
- Kinetic Energy Decay Rates of Supersonic and Super-Alfvénic Turbulence in Star-Forming Clouds (1997) (388)
- The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing (2008) (373)
- SIMULATIONS ON A MOVING MESH: THE CLUSTERED FORMATION OF POPULATION III PROTOSTARS (2011) (330)
- Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence (1999) (311)
- Analyzing Inverse Problems with Invertible Neural Networks (2018) (309)
- MODELING COLLAPSE AND ACCRETION IN TURBULENT GAS CLOUDS: IMPLEMENTATION AND COMPARISON OF SINK PARTICLES IN AMR AND SPH (2010) (302)
- The Formation and Fragmentation of Disks Around Primordial Protostars (2011) (280)
- Molecular Cloud Evolution. II. From Cloud Formation to the Early Stages of Star Formation in Decaying Conditions (2006) (269)
- The Formation of Stellar Clusters: Gaussian Cloud Conditions. II. (1999) (264)
- Modelling CO formation in the turbulent interstellar medium (2009) (255)
- Cluster-formation in the Rosette molecular cloud at the junctions of filaments (2012) (254)
- The Stellar Mass Spectrum from Non-Isothermal Gravoturbulent Fragmentation (2004) (251)
- ON THE STAR FORMATION EFFICIENCY OF TURBULENT MAGNETIZED CLOUDS (2012) (244)
- Formation and evolution of primordial protostellar systems (2012) (240)
- GRAVITATIONAL FRAGMENTATION IN TURBULENT PRIMORDIAL GAS AND THE INITIAL MASS FUNCTION OF POPULATION III STARS (2010) (233)
- A NEW JEANS RESOLUTION CRITERION FOR (M)HD SIMULATIONS OF SELF-GRAVITATING GAS: APPLICATION TO MAGNETIC FIELD AMPLIFICATION BY GRAVITY-DRIVEN TURBULENCE (2011) (229)
- One-Point Probability Distribution Functions of Supersonic Turbulent Flows in Self-gravitating Media (2000) (221)
- Accretion-driven turbulence as universal process: galaxies, molecular clouds, and protostellar disks (2009) (218)
- The Formation of Stellar Clusters: Mass Spectra from Turbulent Molecular Cloud Fragmentation (2001) (203)
- H ii REGIONS: WITNESSES TO MASSIVE STAR FORMATION (2010) (199)
- The SILCC (SImulating the LifeCycle of molecular Clouds) project – I. Chemical evolution of the supernova-driven ISM (2014) (198)
- Clump morphology and evolution in MHD simulations of molecular cloud formation (2008) (194)
- Physical Processes in the Interstellar Medium (2014) (193)
- The first galaxies : assembly, cooling and the onset of turbulence (2008) (186)
- THE FIRST GALAXIES: CHEMICAL ENRICHMENT, MIXING, AND STAR FORMATION (2010) (180)
- From the warm magnetized atomic medium to molecular clouds (2008) (179)
- The First Stellar Cluster (2007) (176)
- Modelling CO emission – I. CO as a column density tracer and the X factor in molecular clouds (2010) (174)
- Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence (2000) (169)
- THE FRACTAL DENSITY STRUCTURE IN SUPERSONIC ISOTHERMAL TURBULENCE: SOLENOIDAL VERSUS COMPRESSIVE ENERGY INJECTION (2007) (160)
- Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster (1997) (160)
- Mach number dependence of turbulent magnetic field amplification: solenoidal versus compressive flows. (2011) (159)
- THE INTERPLAY OF MAGNETIC FIELDS, FRAGMENTATION, AND IONIZATION FEEDBACK IN HIGH-MASS STAR FORMATION (2010) (155)
- The Formation of Stellar Clusters in Turbulent Molecular Clouds: Effects of the Equation of State (2002) (148)
- The Formation of Supermassive Black Holes in the First Galaxies (2010) (147)
- Importance of the Initial Conditions for Star Formation - I. Cloud Evolution and Morphology (2010) (144)
- The SILCC (SImulating the LifeCycle of molecular Clouds) project - II. Dynamical evolution of the supernova-driven ISM and the launching of outflows (2015) (138)
- Small-scale dynamo action during the formation of the first stars and galaxies - I. The ideal MHD limit (2010) (137)
- Collapse, outflows and fragmentation of massive, turbulent and magnetized prestellar barotropic cores (2011) (136)
- CO-dark gas and molecular filaments in Milky Way-type galaxies (2014) (133)
- LIMITING ACCRETION ONTO MASSIVE STARS BY FRAGMENTATION-INDUCED STARVATION (2010) (133)
- A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency: First Tests (2003) (132)
- THE GENERATION OF STRONG MAGNETIC FIELDS DURING THE FORMATION OF THE FIRST STARS (2010) (132)
- The First Supernova Explosions: Energetics, Feedback, and Chemical Enrichment (2007) (127)
- LAUNCHING COSMIC-RAY-DRIVEN OUTFLOWS FROM THE MAGNETIZED INTERSTELLAR MEDIUM (2015) (123)
- TOPoS - II. On the bimodality of carbon abundance in CEMP stars Implications on the early chemical evolution of galaxies (2015) (119)
- Modelling CO emission – II. The physical characteristics that determine the X factor in Galactic molecular clouds (2011) (114)
- On the nature of star-forming filaments – I. Filament morphologies (2014) (113)
- MODELING JET AND OUTFLOW FEEDBACK DURING STAR CLUSTER FORMATION (2014) (107)
- Modelling the supernova-driven ISM in different environments (2014) (107)
- The SILCC project - III. Regulation of star formation and outflows by stellar winds and supernovae (2016) (107)
- THE DELAY OF POPULATION III STAR FORMATION BY SUPERSONIC STREAMING VELOCITIES (2011) (107)
- Magnetic fields during the early stages of massive star formation – I. Accretion and disc evolution (2011) (105)
- Quiescent and Coherent Cores from Gravoturbulent Fragmentation (2003) (105)
- ON THE EVOLUTION OF THE DENSITY PROBABILITY DENSITY FUNCTION IN STRONGLY SELF-GRAVITATING SYSTEMS (2013) (101)
- How long does it take to form a molecular cloud (2012) (100)
- THE SMALL-SCALE DYNAMO AND NON-IDEAL MAGNETOHYDRODYNAMICS IN PRIMORDIAL STAR FORMATION (2012) (99)
- TreeCol: a novel approach to estimating column densities in astrophysical simulations (2011) (99)
- UNDERSTANDING SPATIAL AND SPECTRAL MORPHOLOGIES OF ULTRACOMPACT H ii REGIONS (2010) (97)
- ON THE INITIAL MASS FUNCTION OF LOW-METALLICITY STARS: THE IMPORTANCE OF DUST COOLING (2013) (97)
- HIGH- AND LOW-MASS STAR-FORMING REGIONS FROM HIERARCHICAL GRAVITATIONAL FRAGMENTATION. HIGH LOCAL STAR FORMATION RATES WITH LOW GLOBAL EFFICIENCIES (2009) (95)
- Disc formation in turbulent massive cores: circumventing the magnetic braking catastrophe (2012) (94)
- Dwarf Spheroidal Satellite Galaxies without Dark Matter: Results from Two Different Numerical Techniques (1997) (94)
- The link between molecular cloud structure and turbulence (2010) (92)
- Dynamic Cores in Hydrostatic Disguise (2003) (90)
- THE FIRST GALAXIES: ASSEMBLY WITH BLACK HOLE FEEDBACK (2011) (89)
- Is the scaling of supersonic turbulence universal? (2008) (87)
- Star Formation in Isolated Disk Galaxies. I. Models and Characteristics of Nonlinear Gravitational Collapse (2005) (87)
- Turbulence-induced disc formation in strongly magnetized cloud cores (2013) (86)
- On the nature of star-forming filaments – II. Subfilaments and velocities (2015) (85)
- Evolving structures of star-forming clusters (2005) (85)
- The effects of accretion luminosity upon fragmentation in the early universe (2011) (85)
- The ISM in spiral galaxies: can cooling in spiral shocks produce molecular clouds? (2008) (84)
- MODELING DUST EVOLUTION IN GALAXIES WITH A MULTIPHASE, INHOMOGENEOUS ISM (2016) (84)
- On the Constancy of the Characteristic Mass of Young Stars (2008) (83)
- Algorithmic comparisons of decaying, isothermal, supersonic turbulence (2008) (82)
- A NEW DENSITY VARIANCE–MACH NUMBER RELATION FOR SUBSONIC AND SUPERSONIC ISOTHERMAL TURBULENCE (2012) (82)
- Understanding star formation in molecular clouds - I. Effects of line-of-sight contamination on the column density structure (2014) (78)
- THE TURBULENCE SPECTRUM OF MOLECULAR CLOUDS IN THE GALACTIC RING SURVEY: A DENSITY-DEPENDENT PRINCIPAL COMPONENT ANALYSIS CALIBRATION (2011) (78)
- Winds and radiation in unison: a new semi-analytic feedback model for cloud dissolution (2017) (77)
- The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function (2005) (76)
- Titans of the early Universe: The Prato statement on the origin of the first supermassive black holes (2018) (76)
- Magnetic fields during the early stages of massive star formation – II. A generalized outflow criterion (2011) (76)
- The HI/OH/Recombination line survey of the inner Milky Way (THOR). Survey overview and data release 1 (2016) (75)
- The evolution of supermassive Population III stars (2017) (74)
- Importance of the initial conditions for star formation - III. Statistical properties of embedded protostellar clusters (2011) (74)
- Control of Star Formation in Galaxies by Gravitational Instability (2004) (74)
- Star Formation in Isolated Disk Galaxies. II. Schmidt Laws and Efficiency of Gravitational Collapse (2005) (73)
- On the Maximum Mass of Accreting Primordial Supermassive Stars (2017) (73)
- The first galaxies: signatures of the initial starburst (2009) (72)
- The linewidth-size relationship in the dense ISM of the Central Molecular Zone (2012) (72)
- Clump lifetimes and the initial mass function (2007) (67)
- Importance of the initial conditions for star formation – II. Fragmentation-induced starvation and accretion shielding (2011) (67)
- The SILCC project - IV. Impact of dissociating and ionizing radiation on the interstellar medium and Hα emission as a tracer of the star formation rate (2016) (66)
- THE EFFECT OF DUST COOLING ON LOW-METALLICITY STAR-FORMING CLOUDS (2011) (66)
- Can Protostellar Jets Drive Supersonic Turbulence in Molecular Clouds? (2007) (64)
- Effects of primordial chemistry on the cosmic microwave background (2008) (64)
- Protostellar mass accretion rates from gravoturbulent fragmentation (2004) (62)
- Star formation in galaxy evolution : connecting numerical models to reality (2016) (61)
- Magnetic field amplification by small-scale dynamo action: dependence on turbulence models and Reynolds and Prandtl numbers. (2011) (61)
- Formation of Globular Clusters in Galaxy Mergers (2004) (60)
- The CARMA-NRO Orion Survey (2018) (60)
- Constraining the primordial initial mass function with stellar archaeology (2014) (59)
- Reionization - A probe for the stellar population and the physics of the early universe. (2008) (59)
- SILCC-Zoom: the dynamic and chemical evolution of molecular clouds (2017) (58)
- PHANGS–ALMA: Arcsecond CO(2–1) Imaging of Nearby Star-forming Galaxies (2021) (58)
- GRAVITATIONAL CONTRACTION VERSUS SUPERNOVA DRIVING AND THE ORIGIN OF THE VELOCITY DISPERSION–SIZE RELATION IN MOLECULAR CLOUDS (2015) (56)
- Star Formation at Very Low Metallicity. II. On the Insignificance of Metal-Line Cooling During the Early Stages of Gravitational Collapse (2005) (55)
- Chemical mixing in smoothed particle hydrodynamics simulations (2008) (55)
- EFFECTS OF VARYING THE THREE-BODY MOLECULAR HYDROGEN FORMATION RATE IN PRIMORDIAL STAR FORMATION (2010) (55)
- Understanding star formation in molecular clouds: II. Signatures of gravitational collapse of IRDCs (2014) (54)
- Magnetic field amplification during gravitational collapse - Influence of initial conditions on dynamo evolution and saturation (2012) (53)
- The complex distribution of recently formed stars. Bimodal stellar clustering in the star-forming region NGC 346 (2014) (53)
- A theoretical explanation for the Central Molecular Zone asymmetry (2017) (53)
- Draco: A Failure of the Tidal Model (2003) (51)
- LINE PROFILES OF CORES WITHIN CLUSTERS. II. SIGNATURES OF DYNAMICAL COLLAPSE DURING HIGH-MASS STAR FORMATION (2013) (51)
- The star formation efficiency and its relation to variations in the initial mass function (2008) (51)
- ON THE TEMPERATURE STRUCTURE OF THE GALACTIC CENTER CLOUD G0.253+0.016 (2013) (51)
- TOPoS. IV. Chemical abundances from high-resolution observations of seven extremely metal-poor stars (2018) (51)
- Descendants of the first stars: the distinct chemical signature of second-generation stars (2018) (50)
- STAR FORMATION AT VERY LOW METALLICITY. IV. FRAGMENTATION DOES NOT DEPEND ON METALLICITY FOR COLD INITIAL CONDITIONS (2007) (50)
- Detection of two power-law tails in the probability distribution functions of massive GMCs (2015) (50)
- THE INFLUENCE OF MAGNETIC FIELDS ON THE THERMODYNAMICS OF PRIMORDIAL STAR FORMATION (2009) (49)
- The observational signature of the first H ii regions (2009) (48)
- The Molecular Cloud Lifecycle (2020) (48)
- The formation of direct collapse black holes under the influence of streaming velocities (2017) (48)
- Magnetic Field Amplification in Young Galaxies (2013) (48)
- STAR FORMATION AT VERY LOW METALLICITY. V. THE GREATER IMPORTANCE OF INITIAL CONDITIONS COMPARED TO METALLICITY THRESHOLDS (2008) (47)
- Distances to PHANGS Galaxies: New Tip of the Red Giant Branch Measurements and Adopted Distances (2020) (47)
- Rotation and internal structure of Population III protostars (2012) (46)
- DISTRIBUTION AND MASS OF DIFFUSE AND DENSE CO GAS IN THE MILKY WAY (2016) (46)
- GRAPESPH with fully periodic boundary conditions: fragmentation of molecular clouds (1997) (46)
- TOPoS: I. Survey design and analysis of the first sample (2013) (45)
- The influence of streaming velocities on the formation of the first stars (2018) (45)
- On the formation of very metal-poor stars: The case of SDSS J1029151+172927 (2012) (45)
- Variable accretion rates and fluffy first stars (2011) (45)
- Galactic Supernova Remnant Candidates Discovered by THOR (2017) (45)
- Molecular Cloud Turbulence and Star Formation (2006) (44)
- Exploring the nature of the Lyman-α emitter CR7 (2015) (44)
- Protostellar angular momentum evolution during gravoturbulent fragmentation (2004) (43)
- Modeling H2 formation in the turbulent ISM: Solenoidal versus compressive turbulent forcing (2011) (43)
- LINE PROFILES OF CORES WITHIN CLUSTERS. I. THE ANATOMY OF A FILAMENT (2012) (43)
- The First Million Years of the Sun: A Calculation of the Formation and Early Evolution of a Solar Mass Star (2001) (43)
- The 12CO/13CO ratio in turbulent molecular clouds (2014) (43)
- Saturation of the turbulent dynamo. (2015) (42)
- About the morphology of dwarf spheroidal galaxies and their dark matter content (2002) (41)
- Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies (2017) (41)
- Statistical properties of supersonic turbulence in the Lagrangian and Eulerian frameworks (2011) (41)
- THE CO-TO-H2 CONVERSION FACTOR ACROSS THE PERSEUS MOLECULAR CLOUD (2014) (41)
- THOR: The H I, OH, Recombination line survey of the Milky Way. The pilot study: H I observations of the giant molecular cloud W43 (2015) (40)
- The Formation of Stellar Clusters: Time-Varying Protostellar Accretion Rates (2001) (40)
- Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X (2015) (39)
- Formation of massive seed black holes via collisions and accretion (2018) (39)
- On the structure of self-gravitating molecular clouds (2001) (39)
- Probing high-redshift quasars with ALMA. I. Expected observables and potential number of sources (2010) (38)
- warpfield2.0: feedback-regulated minimum star formation efficiencies of giant molecular clouds (2018) (38)
- Numerical Star-Formation Studies - A Status Report (2009) (38)
- Predicting the locations of possible long-lived low-mass first stars: importance of satellite dwarf galaxies (2017) (37)
- Collisions in primordial star clusters (2018) (36)
- Protostellar collapse and fragmentation using an MHD gadget (2010) (36)
- MODEST-1: Integrating stellar evolution and stellar dynamics (2002) (36)
- INFLUENCE OF PRIMORDIAL MAGNETIC FIELDS ON 21 CM EMISSION (2008) (36)
- Accretion and magnetic field morphology around Class 0 stage protostellar discs (2014) (35)
- Equilibrium initialization and stability of three-dimensional gas discs (2010) (35)
- COLLECTIVE OUTFLOW FROM A SMALL MULTIPLE STELLAR SYSTEM (2014) (35)
- Dark stars: Implications and constraints from cosmic reionization and extragalactic background radiation (2008) (34)
- Diffusion in supersonic turbulent compressible flows. (2003) (34)
- 3D continuum radiative transfer in complex dust configurations. II. 3D structure of the dense molecular cloud core ρ Oph D (2005) (34)
- Nuclear spirals in the inner Milky Way (2017) (34)
- PHANGS–ALMA Data Processing and Pipeline (2021) (33)
- Lyman–Werner UV escape fractions from primordial haloes (2015) (33)
- Indications of a sub-linear and non-universal Kennicutt-Schmidt relationship (2013) (33)
- FLICKERING OF 1.3 cm SOURCES IN SGR B2: TOWARD A SOLUTION TO THE ULTRACOMPACT H ii REGION LIFETIME PROBLEM (2013) (32)
- MODEST-2: a summary (2003) (32)
- THE IMPACT OF THERMODYNAMICS ON GRAVITATIONAL COLLAPSE: FILAMENT FORMATION AND MAGNETIC FIELD AMPLIFICATION (2012) (32)
- Turbulent mixing in the interstellar medium: an application for Lagrangian tracer particles (2008) (32)
- Simulations of the star-forming molecular gas in an interacting M51-like galaxy: cloud population statistics (2019) (31)
- Continuum sources from the THOR survey between 1 and 2 GHz (2016) (31)
- Fervent: chemistry-coupled, ionizing and non-ionizing radiative feedback in hydrodynamical simulations (2015) (31)
- The reliability of approximate radiation transport methods for irradiated disk studies (2013) (31)
- Molecular Gas Properties on Cloud Scales across the Local Star-forming Galaxy Population (2020) (31)
- Numerical and semi-analytic core mass distributions in supersonic isothermal turbulence (2010) (31)
- Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC (2015) (31)
- Star Formation in Molecular Clouds (2011) (30)
- HIERARCHICAL STELLAR STRUCTURES IN THE LOCAL GROUP DWARF GALAXY NGC 6822 (2010) (30)
- THE CLUSTERING BEHAVIOR OF PRE-MAIN-SEQUENCE STARS IN NGC 346 IN THE SMALL MAGELLANIC CLOUD (2008) (30)
- The role of stellar collisions for the formation of massive stars (2010) (30)
- Simulations of the Milky Way’s central molecular zone – I. Gas dynamics (2020) (30)
- A quantification of the non-spherical geometry and accretion of collapsing cores (2010) (30)
- Feeding versus Falling: The Growth and Collapse of Molecular Clouds in a Turbulent Interstellar Medium (2017) (30)
- Gravity or turbulence? IV. Collapsing cores in out-of-virial disguise (2017) (29)
- How well does CO emission measure the H2 mass of MCs (2016) (29)
- Simulations of the Milky Way’s Central Molecular Zone – II. Star formation (2020) (29)
- How an improved implementation of H2 self-shielding influences the formation of massive stars and black holes (2015) (29)
- The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces (2019) (28)
- The PHANGS-MUSE survey. Probing the chemo-dynamical evolution of disc galaxies (2021) (27)
- WIMP DM and first stars: suppression of fragmentation in primordial star formation (2012) (27)
- A dynamical mechanism for the origin of nuclear rings (2018) (27)
- The Physics of Star Cluster Formation and Evolution (2020) (27)
- On the Rotation of Supermassive Stars (2017) (26)
- FirstLight II: Star formation rates of primeval galaxies from z=5-15 (2018) (26)
- Stellar and substellar initial mass function: a model that implements gravoturbulent fragmentation and accretion (2010) (26)
- Using CO line ratios to trace the physical properties of molecular clouds (2016) (26)
- A simple method to convert sink particles into stars (2016) (26)
- A New Statistical Model for Population III Supernova Rates: Discriminating Between ΛCDM and WDM Cosmologies (2016) (26)
- Small-scale dynamo at low magnetic Prandtl numbers. (2012) (26)
- Histogram of oriented gradients: a technique for the study of molecular cloud formation (2018) (26)
- Radio continuum emission in the northern Galactic plane: Sources and spectral indices from the THOR survey (Corrigendum) (2018) (25)
- Forming clusters within clusters: how 30 Doradus recollapsed and gave birth again (2017) (24)
- The HI/OH/Recombination line survey of the inner Milky Way (THOR): data release 2 and H I overview (2019) (24)
- Radial gas motions in The H i Nearby Galaxy Survey (THINGS) (2016) (24)
- Physical Processes in Star Formation (2020) (24)
- The SILCC project – V. The impact of magnetic fields on the chemistry and the formation of molecular clouds (2018) (24)
- Hierarchical star formation across the grand-design spiral NGC 1566 (2017) (24)
- The sonic scale of interstellar turbulence (2021) (24)
- On the indeterministic nature of star formation on the cloud scale (2018) (23)
- Lyman-Werner escape fractions from the first galaxies (2017) (23)
- FirstLight III: rest-frame UV-optical spectral energy distributions of simulated galaxies at cosmic dawn (2018) (23)
- Accelerating astrophysical particle simulations with programmable hardware (FPGA and GPU) (2009) (23)
- On the duration of the embedded phase of star formation (2020) (23)
- Mach number study of supersonic turbulence: the properties of the density field (2015) (23)
- The stellar mass spectrum in warm and dusty gas: deviations from Salpeter in the Galactic centre and in circumnuclear starburst regions (2006) (23)
- Formation of the First Stars and Black Holes (2020) (22)
- Interpreting the sub-linear Kennicutt–Schmidt relationship: the case for diffuse molecular gas (2014) (22)
- Magnetic fields in star-forming systems (I): idealized synthetic signatures of dust polarization and Zeeman splitting in filaments (2018) (22)
- From parallel to perpendicular – On the orientation of magnetic fields in molecular clouds (2020) (22)
- The reliability of observational measurements of column density probability distribution functions (2016) (22)
- Line profiles of cores within clusters – III. What is the most reliable tracer of core collapse in dense clusters? (2014) (22)
- Collisional N-body Dynamics Coupled to Self-gravitating Magnetohydrodynamics Reveals Dynamical Binary Formation (2019) (21)
- How the First Stars Regulated Star Formation. II. Enrichment by Nearby Supernovae (2016) (21)
- A NEW APPROACH TO DETERMINE OPTICALLY THICK H2 COOLING AND ITS EFFECT ON PRIMORDIAL STAR FORMATION (2014) (21)
- From Diffuse Gas to Dense Molecular Cloud Cores (2020) (21)
- The origin of dust polarization in molecular outflows (2017) (21)
- The IMF as a function of supersonic turbulence (2016) (21)
- Cloud formation in colliding flows: influence of the choice of cooling function (2013) (21)
- CO line ratios in molecular clouds: the impact of environment (2017) (21)
- EVIDENCE OF SHORT TIMESCALE FLUX DENSITY VARIATIONS OF UC H II REGIONS IN SGR B2 MAIN AND NORTH (2015) (21)
- III. An ultra iron-poor multiple CEMP system ? (2016) (20)
- Molecular line emission in NGC 4945, imaged with ALMA (2018) (20)
- The PHANGS-HST Survey: Physics at High Angular Resolution in Nearby Galaxies with the Hubble Space Telescope (2021) (20)
- Ubiquitous velocity fluctuations throughout the molecular interstellar medium (2020) (19)
- Observational constraints on the survival of pristine stars (2019) (19)
- Giant molecular cloud catalogues for PHANGS-ALMA: methods and initial results (2021) (19)
- Low-metallicity star formation: relative impact of metals and magnetic fields (2014) (19)
- ARE MOLECULAR OUTFLOWS AROUND HIGH-MASS STARS DRIVEN BY IONIZATION FEEDBACK? (2012) (19)
- Astrophysical particle simulations with large custom GPU clusters on three continents (2011) (19)
- Adaptive mesh refinement simulations of a galaxy cluster merger – I. Resolving and modelling the turbulent flow in the cluster outskirts (2017) (19)
- The PHANGS–JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS (2022) (19)
- IMPACT OF SUPERNOVA AND COSMIC-RAY DRIVING ON THE SURFACE BRIGHTNESS OF THE GALACTIC HALO IN SOFT X-RAYS (2015) (18)
- Spectral shifting strongly constrains molecular cloud disruption by radiation pressure on dust (2017) (18)
- Synthetic [C ii] emission maps of a simulated molecular cloud in formation (2018) (18)
- The geometry of the gas surrounding the Central Molecular Zone: on the origin of localized molecular clouds with extreme velocity dispersions (2019) (18)
- Formation sites of Population III star formation: The effects of different levels of rotation and turbulence on the fragmentation behaviour of primordial gas (2019) (17)
- When H ii regions are complicated: considering perturbations from winds, radiation pressure, and other effects (2019) (17)
- Simulating the UV escape fractions from molecular cloud populations in star-forming dwarf and spiral galaxies (2017) (17)
- Are Dwarf Spheroidal Galaxies Dark Matter Dominated or Remnants of Disrupted Larger Satellite Galaxies? A Possible Test (2001) (17)
- Synthetic observations of molecular clouds in a galactic centre environment – I. Studying maps of column density and integrated intensity (2015) (17)
- Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey (2018) (17)
- Metallicity evolution of direct collapse black hole hosts: CR7 as a case study (2017) (17)
- Measuring the mixing scale of the ISM within nearby spiral galaxies (2020) (16)
- GALACTIC SYNCHROTRON EMISSION AND THE FAR-INFRARED–RADIO CORRELATION AT HIGH REDSHIFT (2016) (16)
- Low-J CO Line Ratios from Single-dish CO Mapping Surveys and PHANGS-ALMA (2021) (16)
- The (Un)predictability of Star Formation on a Cloud Scale (2018) (16)
- Detecting strongly lensed supernovae at z ∼ 5–7 with LSST (2018) (15)
- Relations between Molecular Cloud Structure Sizes and Line Widths in the Large Magellanic Cloud (2019) (15)
- Stellar structures, molecular gas, and star formation across the PHANGS sample of nearby galaxies (2021) (15)
- Star formation efficiencies of molecular clouds in a galactic centre environment (2015) (15)
- Statistical properties of dark matter mini-haloes at z ≥ 15 (2014) (15)
- A survey for hydroxyl in the THOR pilot region around W43 (2015) (15)
- WARPFIELD-EMP: The self-consistent prediction of emission lines from evolving H ii regions in dense molecular clouds (2019) (15)
- A minimum dilution scenario for supernovae and consequences for extremely metal-poor stars (2020) (15)
- ULTRAVIOLET ESCAPE FRACTIONS FROM GIANT MOLECULAR CLOUDS DURING EARLY CLUSTER FORMATION (2016) (15)
- Statistical analysis of the mass-to-flux ratio in turbulent cores: effects of magnetic field reversals and dynamo amplification (2011) (14)
- The Decay of Supersonic and Super-Alfvénic Turbulence in Star-Forming Clouds (1998) (14)
- Massive star formation by accretion II. Rotation: how to circumvent the angular momentum barrier? (2017) (14)
- Strong Excess Faraday Rotation on the Inside of the Sagittarius Spiral Arm (2019) (14)
- SIGNALS: I. Survey description (2019) (14)
- Periodicity makes galactic shocks unstable – I. Linear analysis (2017) (14)
- Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies (2020) (14)
- Modeling of the Effects of Stellar Feedback during Star Cluster Formation Using a Hybrid Gas and N-Body Method (2020) (14)
- 3D Continuum radiative transfer in complex dust configurations around young stellar objects and active nuclei II. 3D Structure of the dense molecular cloud core Rho Oph D (2004) (13)
- Ionization front-driven turbulence in the clumpy interstellar medium (2008) (13)
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- P o S ( N I C X I I I ) 0 5 3 The first generations of stars (2015) (0)
- Volatiles in Protoplanetary Disks The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters (2014) (0)
- Statistical properties of dark matter mini-halos (2012) (0)
- Detecting the First Quasars with ALMA (2009) (0)
- Fervent: Chemistry-coupled, ionising and non-ionising radiative feedback in magnetohydrodynamical simulations (2021) (0)
- Molecular Lines from Self-gravitating Turbulent Clouds (2003) (0)
- Erratum: Gravity or turbulence? - IV. Collapsing cores in out of virial disguise (2019) (0)
- Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II (2022) (0)
- Can Magnetized Turbulence Support Molecular Clouds (2000) (0)
- The mechanical alignment of dust (MAD). I. The spin-up process of fractal grains by a gas-dust drift (2022) (0)
- The CARMA-NRO Orion Survey-Filamentary structure as seen in C18O emission (2019) (0)
- Assessing the influence of metallicity on fragmentation of proto-galactic gas (2006) (0)
- Continuum radiative transfer in complex dust configurations around young stellar objects and active nuclei II . 3 D Structure of the dense molecular cloud core ρ Oph (2004) (0)
- Studying the star formation efficiency of cloud collisions and gravo-turbulent fragmentation (2007) (0)
- VizieR Online Data Catalog: 4 molecular clouds SPIRE 250um maps (Schneider+, 2015) (2015) (0)
- Formation of massive black holes via collisions and accretion (2018) (0)
- The Stellar IMF in Low‐Metallicity Gas (2010) (0)
- Galactic-scale star formation by gravitational instability (2006) (0)
- The Effect of Environment on Massive Star Formation (2010) (0)
- Formation of metal-free binaries: Impact of H2 line cooling and CIE cooling (2022) (0)
- The Physics of Star Cluster Formation and Evolution (2020) (0)
- PHANGS--JWST First Results: ISM structure on the turbulent Jeans scale in four disk galaxies observed by JWST and ALMA (2022) (0)
- Detecting the first quasars with ALMA (2009) (0)
- 3D continuum radiative transfer in complex dust configurations-II. 3D structure of the dense molecular cloud core $\mathsf{\rho}$ Oph D (2008) (0)
- STRUCTURES – a unifying approach to emergent phenomena in the physical world, mathematics, and complex data (2018) (0)
- The $^{12}\textrm{CO}/^{13}\textrm{CO}$ ratio in turbulent molecular clouds (2014) (0)
- Measuring Young Stars in Space and Time. II. The Pre-main-sequence Stellar Content of N44 (2020) (0)
- Flux Density Variations and Radio Recombination Line Emission at 7 mm and 3.6 cm in W49A (2019) (0)
- Hubble Tarantula Treasury Project (2018) (0)
- Star Formation and ISM Dynamics on Galactic Disk Scales (2017) (0)
- THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar / planetary evolution and molecular clouds (2015) (0)
- style emulateapj v . 11 / 10 / 09 THE FIRST GALAXIES : CHEMICAL ENRICHMENT , MIXING , AND STAR FORMATION (2010) (0)
- Density distribution function of a self-gravitating isothermal turbulent fluid in the context of molecular cloud ensembles – III. Virial analysis (2022) (0)
- Resolved stellar population properties of PHANGS-MUSE galaxies (2023) (0)
- A Model for Dwarf Spheroidal Satellite Galaxies without Dark Matter (1998) (0)
- Black hole feedback on the first galaxies (2012) (0)
- From dark matter halos to pre-stellar cores: High resolution follow-up of cosmological Lyman-Werner simulations (2023) (0)
- Influence of magnetic field and stellar radiative feedback on the collapse and the stellar mass spectrum of a massive star-forming clump (2022) (0)
- 30 Doradus, the double stellar birth scenario by $N$-body \&\textsc{warpfield} clouds (2022) (0)
- Physical Processes in Star Formation (2020) (0)
- Modelling the formation of two stellar generations in massive star clusters: the case of 30 Doradus (2023) (0)
- Magnetic fields in the first galaxies: Dynamo amplification and limits from reionization (2011) (0)
- Optimal neighbourhood to nurture giants (2019) (0)
- The importance of initial conditions and metallicity for the fragmentation of protogalactic gas (2009) (0)
- Importance of Thermodynamics for Fragmentation and Star Formation (2008) (0)
- The density distribution and physical origins of intermittency in supersonic, highly magnetised turbulence with diverse modes of driving (2021) (0)
- Small-scale dynamo action in primordial halos (2012) (0)
- Spectral classification of young stars using conditional invertible neural networks. I. Introducing and validating the method (2023) (0)
- The impact of streaming velocities: delaying the formation of the rst stars (2018) (0)
- From Diffuse Gas to Dense Molecular Cloud Cores (2020) (0)
- Star Formation Laws and Efficiencies across 80 Nearby Galaxies (2023) (0)
- Massive star formation by accretion: how to circumvent the angular momentum barrier? (2017) (0)
- PHANGS–MUSE: The H ii region luminosity function of local star-forming galaxies (2021) (0)
- Magnetic Field Generation During the Formation of the First Stars (2012) (0)
- The role of magnetic fields during primordial star formation (2011) (0)
- A Model for the Saturation of the Turbulent Dynamo (2015) (0)
- Signatures of Dynamical Collapse during High-Mass Star Formation (2013) (0)
- Primordial Magnetic Fields: Reionization Constraints and Implications for the First Stars (2010) (0)
- Simulating the chemistry and dynamics of molecular clouds (2009) (0)
- Formation of Stellar Clusters and the Importance of Thermodynamics for Fragmentation (2007) (0)
- B-fields do not suppress star formation in low metallicity dwarf galaxies (0)
- A Dynamic Formation Channel for Binaries in Embedded Clusters (2019) (0)
- Fragmentation of Molecular Clouds II: The Standard Model (1999) (0)
- Probing the Hierarchy in Stellar Clustering (2015) (0)
- Ubiquitous velocity fluctuations throughout the molecular interstellar medium (2020) (0)
- Community paper „The Early Universe from Inflation to Reionization“ (2016) (0)
- Serendipitous Nebular-phase JWST Imaging of SN Ia SN 2021aefx: Testing the Confinement of 56Co Decay Energy (2023) (0)
- Modeling the effects of turbulence in zero- and low-metallicity star formation (2011) (0)
- Tracing star formation with radio emission (2017) (0)
- Fractal Density Distribution of Interstellar Clouds from Numerical Simulations of Compressively Driven Supersonic Turbulence (2007) (0)
- The physical origin of super-competitive accretion during the formation of the first supermassive black holes (2023) (0)
- C i and CO in nearby spiral galaxies. I. Line ratio and abundance variations at ~200 pc scales (2022) (0)
- Population III X-ray binaries and their impact on the early universe (2023) (0)
- A model for the infrared-radio correlation of main-sequence galaxies at GHz frequencies and its dependence on redshift and stellar mass (2022) (0)
- P o S ( C R F 2 0 1 0 ) 0 2 7 Magnetic fields during primordial star formation (2011) (0)
- High Resolution VLA Continuum and Radio Recombination Line Emission in W49A (2020) (0)
- Constraints on the dark matter clumping factor and halo profiles from the cosmic gamma-ray background (2008) (0)
- Stellar associations powering H ii regions – I. Defining an evolutionary sequence (2023) (0)
- Radio Recombination Line Observations of Flickering Ultracompact HII Regions (2015) (0)
- Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties (2023) (0)
- Variable accretion rates and fluffy first stars (2012) (0)
- Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50 (2022) (0)
- Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies (2022) (0)
- The Effect of Dust Cooling in the Fragmentation of Star‐Forming Clouds (2010) (0)
- Timescales in supersonic turbulence (2015) (0)
- Dark matter annihilation feedback: Effects upon collapse and fragmentation (2012) (0)
- Dynamic UC HII regions in Sgr B2: Flickering and Ionized Flows (2013) (0)
- GRAVITATIONAL INSTABILITY IN GALACTIC DISKS: INITIAL CONDITIONS FOR STAR FORMATION.Mordecai- (2005) (0)
- Dynamic cores in hydrostatic disguise. II. "Coherent" cores from turbulent fragmentation (2003) (0)
- Globular Cluster Formation in Galaxy Mergers (2005) (0)
- Jet Driven Turbulence (2009) (0)
- Non-Isothermal Gravoturbulent Fragmentation (2005) (0)
- Early-forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly (2022) (0)
- CARMA-NRO Orion Survey: Unbiased Survey of Dense Cores and Core Mass Functions in Orion A (2022) (0)
- Hydrodynamical and MHD turbulent support against gravitational collapse. (1999) (0)
- Gangotri Wave—A High Density Gas Ripple in the Inner Galaxy (2022) (0)
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