| 1 | Mapping the magnetic field in the Taurus/B211 filamentary cloud with SOFIA HAWC + and comparing with simulation | 3.3 | 42 | Citations (PDF) |
| 2 | Magnetic fields in the formation of the first stars – II. Results | 3.3 | 37 | Citations (PDF) |
| 3 | Infrared dust echoes from neutron star mergers | 3.3 | 9 | Citations (PDF) |
| 4 | ORION2: A magnetohydrodynamics code for star formation | 1.5 | 15 | Citations (PDF) |
| 5 | Magnetic fields in the formation of the first stars – I. Theory versus simulation | 3.3 | 50 | Citations (PDF) |
| 6 | Massive Warm/Hot Galaxy Coronae. II. Isentropic Model | 3.6 | 72 | Citations (PDF) |
| 7 | How do bound star clusters form? | 3.3 | 53 | Citations (PDF) |
| 8 | Star Clusters Across Cosmic Time | 22.4 | 619 | Citations (PDF) |
| 9 | Effect of angular momentum alignment and strong magnetic fields on the formation of protostellar discs | 3.3 | 49 | Citations (PDF) |
| 10 | Dark Matter that Interacts with Baryons: Density Distribution within the Earth and New Constraints on the Interaction Cross-section | 3.6 | 43 | Citations (PDF) |
| 11 | Formation of stellar clusters in magnetized, filamentary infrared dark clouds | 3.3 | 54 | Citations (PDF) |
| 12 | The effects of magnetic fields and protostellar feedback on low-mass cluster formation | 3.3 | 71 | Citations (PDF) |
| 13 | The Supernova Rate beyond the Optical Radius | 7.2 | 8 | Citations (PDF) |
| 14 | The high-mass slope of the IMF | 3.3 | 8 | Citations (PDF) |
| 15 | MASSIVE WARM/HOT GALAXY CORONAE AS PROBED BY UV/X-RAY OXYGEN ABSORPTION AND EMISSION. I. BASIC MODEL | 3.6 | 139 | Citations (PDF) |
| 16 | Moving-mesh Simulations of Star-forming Cores in Magneto-gravo-turbulence | 3.6 | 83 | Citations (PDF) |
| 17 | Chemistry and radiative shielding in star-forming galactic discs | 3.3 | 53 | Citations (PDF) |
| 18 | Bondi–Hoyle accretion in a turbulent, magnetized medium | 3.3 | 9 | Citations (PDF) |
| 19 | An unstable truth: how massive stars get their mass | 3.3 | 116 | Citations (PDF) |
| 20 | What physics determines the peak of the IMF? Insights from the structure of cores in radiation-magnetohydrodynamic simulations | 3.3 | 45 | Citations (PDF) |
| 21 | Magnetized interstellar molecular clouds – I. Comparison between simulations and Zeeman observations | 3.3 | 77 | Citations (PDF) |
| 22 | The CH+abundance in turbulent, diffuse molecular clouds | 3.3 | 27 | Citations (PDF) |
| 23 | The turbulent origin of spin–orbit misalignment in planetary systems | 3.3 | 115 | Citations (PDF) |
| 24 | STARS, GAS, AND DARK MATTER IN THE SOLAR NEIGHBORHOOD | 3.6 | 257 | Citations (PDF) |
| 25 | Star cluster formation in turbulent, magnetized dense clumps with radiative and outflow feedback | 3.3 | 117 | Citations (PDF) |
| 26 | BONDI-HOYLE ACCRETION IN AN ISOTHERMAL MAGNETIZED PLASMA | 3.6 | 36 | Citations (PDF) |
| 27 | THE FRAGMENTATION OF MAGNETIZED, MASSIVE STAR-FORMING CORES WITH RADIATIVE FEEDBACK | 3.6 | 164 | Citations (PDF) |
| 28 | INTERSTELLAR H2O MASERS FROM J SHOCKS | 3.6 | 78 | Citations (PDF) |
| 29 | RADIATION TRANSFER OF MODELS OF MASSIVE STAR FORMATION. II. EFFECTS OF THE OUTFLOW | 3.6 | 35 | Citations (PDF) |
| 30 | ULTRA-COMPACT HIGH VELOCITY CLOUDS AS MINIHALOS AND DWARF GALAXIES | 3.6 | 40 | Citations (PDF) |
| 31 | A MASSIVE PROTOSTAR FORMING BY ORDERED COLLAPSE OF A DENSE, MASSIVE CORE | 3.6 | 31 | Citations (PDF) |
| 32 | PHOTOMETRIC REDSHIFTS OF SUBMILLIMETER GALAXIES | 3.6 | 7 | Citations (PDF) |
| 33 | RADIATION-HYDRODYNAMIC SIMULATIONS OF THE FORMATION OF ORION-LIKE STAR CLUSTERS. II. THE INITIAL MASS FUNCTION FROM WINDS, TURBULENCE, AND RADIATION | 3.6 | 194 | Citations (PDF) |
| 34 | A UNIVERSAL, LOCAL STAR FORMATION LAW IN GALACTIC CLOUDS, NEARBY GALAXIES, HIGH-REDSHIFT DISKS, AND STARBURSTS | 3.6 | 470 | Citations (PDF) |
| 35 | AMBIPOLAR DIFFUSION HEATING IN TURBULENT SYSTEMS | 3.6 | 25 | Citations (PDF) |
| 36 | FEEDBACK EFFECTS ON LOW-MASS STAR FORMATION | 3.6 | 88 | Citations (PDF) |
| 37 | RADIATIVELY EFFICIENT MAGNETIZED BONDI ACCRETION | 3.6 | 20 | Citations (PDF) |
| 38 | A STABLE, ACCURATE METHODOLOGY FOR HIGH MACH NUMBER, STRONG MAGNETIC FIELD MHD TURBULENCE WITH ADAPTIVE MESH REFINEMENT: RESOLUTION AND REFINEMENT STUDIES | 3.6 | 55 | Citations (PDF) |
| 39 | SUB-ALFVÉNIC NON-IDEAL MAGNETOHYDRODYNAMIC TURBULENCE SIMULATIONS WITH AMBIPOLAR DIFFUSION. III. IMPLICATIONS FOR OBSERVATIONS AND TURBULENT ENHANCEMENT | 3.6 | 15 | Citations (PDF) |
| 40 | OBSERVING SIMULATED PROTOSTARS WITH OUTFLOWS: HOW ACCURATE ARE PROTOSTELLAR PROPERTIES INFERRED FROM SEDs? | 3.6 | 51 | Citations (PDF) |
| 41 | METALLICITY AND THE UNIVERSALITY OF THE INITIAL MASS FUNCTION | 3.6 | 49 | Citations (PDF) |
| 42 | THE PROTOSTELLAR LUMINOSITY FUNCTION | 3.6 | 117 | Citations (PDF) |
| 43 | THE GLOBAL EVOLUTION OF GIANT MOLECULAR CLOUDS. II. THE ROLE OF ACCRETION | 3.6 | 112 | Citations (PDF) |
| 44 | WHICH PHASE OF THE INTERSTELLAR MEDIUM CORRELATES WITH THE STAR FORMATION RATE? | 3.6 | 151 | Citations (PDF) |
| 45 | AN INITIAL MASS FUNCTION FOR INDIVIDUAL STARS IN GALACTIC DISKS. I. CONSTRAINING THE SHAPE OF THE INITIAL MASS FUNCTION | 3.6 | 55 | Citations (PDF) |
| 46 | ANISOTROPY LENGTHENS THE DECAY TIME OF TURBULENCE IN MOLECULAR CLOUDS | 3.6 | 12 | Citations (PDF) |
| 47 | IRAS 15099–5856: REMARKABLE MID-INFRARED SOURCE WITH PROMINENT CRYSTALLINE SILICATE EMISSION EMBEDDED IN THE SUPERNOVA REMNANT MSH15–52 | 3.6 | 13 | Citations (PDF) |
| 48 | RADIATION-HYDRODYNAMIC SIMULATIONS OF MASSIVE STAR FORMATION WITH PROTOSTELLAR OUTFLOWS | 3.6 | 142 | Citations (PDF) |
| 49 | RADIATION-HYDRODYNAMIC SIMULATIONS OF THE FORMATION OF ORION-LIKE STAR CLUSTERS. I. IMPLICATIONS FOR THE ORIGIN OF THE INITIAL MASS FUNCTION | 3.6 | 121 | Citations (PDF) |
| 50 | THE PROTOSTELLAR MASS FUNCTION | 3.6 | 46 | Citations (PDF) |
| 51 | THE ATOMIC-TO-MOLECULAR TRANSITION IN GALAXIES. III. A NEW METHOD FOR DETERMINING THE MOLECULAR CONTENT OF PRIMORDIAL AND DUSTY CLOUDS | 3.6 | 163 | Citations (PDF) |
| 52 | RADIATION FEEDBACK, FRAGMENTATION, AND THE ENVIRONMENTAL DEPENDENCE OF THE INITIAL MASS FUNCTION | 3.6 | 99 | Citations (PDF) |
| 53 | THE DARK MOLECULAR GAS | 3.6 | 633 | Citations (PDF) |
| 54 | METAL-ION ABSORPTION IN CONDUCTIVELY EVAPORATING CLOUDS | 3.6 | 46 | Citations (PDF) |
| 55 | REGULATION OF STAR FORMATION RATES IN MULTIPHASE GALACTIC DISKS: A THERMAL/DYNAMICAL EQUILIBRIUM MODEL | 3.6 | 373 | Citations (PDF) |
| 56 | SUB-ALFVÉNIC NON-IDEAL MHD TURBULENCE SIMULATIONS WITH AMBIPOLAR DIFFUSION. II. COMPARISON WITH OBSERVATION, CLUMP PROPERTIES, AND SCALING TO PHYSICAL UNITS | 3.6 | 65 | Citations (PDF) |
| 57 | THE STAR FORMATION LAW IN ATOMIC AND MOLECULAR GAS | 3.6 | 384 | Citations (PDF) |
| 58 | THE ATOMIC-TO-MOLECULAR TRANSITION IN GALAXIES. II: H I AND H2COLUMN DENSITIES | 3.6 | 418 | Citations (PDF) |
| 59 | THE EFFECTS OF RADIATIVE TRANSFER ON LOW-MASS STAR FORMATION | 3.6 | 285 | Citations (PDF) |
| 60 | The formation of the first stars and galaxies | 31.3 | 323 | Citations (PDF) |
| 61 | A minimum column density of 1 g cm-2 for massive star formation | 31.3 | 301 | Citations (PDF) |
| 62 | Far‐Infrared Spectral Energy Distributions and Photometric Redshifts of Dusty Galaxies | 3.6 | 19 | Citations (PDF) |
| 63 | Driven and Decaying Turbulence Simulations of Low‐Mass Star Formation: From Clumps to Cores to Protostars | 3.6 | 102 | Citations (PDF) |
| 64 | The Formation of the First Stars. II. Radiative Feedback Processes and Implications for the Initial Mass Function | 3.6 | 232 | Citations (PDF) |
| 65 | THE KINEMATICS OF MOLECULAR CLOUD CORES IN THE PRESENCE OF DRIVEN AND DECAYING TURBULENCE: COMPARISONS WITH OBSERVATIONS | 3.7 | 47 | Citations (PDF) |
| 66 | A Massive-Star-forming Infrared Loop around the Crab-like Supernova Remnant G54.1+0.3: Post-Main-Sequence Triggered Star Formation? | 3.6 | 41 | Citations (PDF) |
| 67 | Sub‐Alfvénic Nonideal MHD Turbulence Simulations with Ambipolar Diffusion. I. Turbulence Statistics | 3.6 | 60 | Citations (PDF) |
| 68 | The Atomic‐to‐Molecular Transition in Galaxies. I. An Analytic Approximation for Photodissociation Fronts in Finite Clouds | 3.6 | 200 | Citations (PDF) |
| 69 | Equations and Algorithms for Mixed‐frame Flux‐limited Diffusion Radiation Hydrodynamics | 3.6 | 141 | Citations (PDF) |
| 70 | Radiation‐Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores | 3.6 | 340 | Citations (PDF) |
| 71 | Molecular Line Emission from Massive Protostellar Disks: Predictions for ALMA and EVLA | 3.6 | 68 | Citations (PDF) |
| 72 | Reconstructing Deconstruction: High‐Velocity Cloud Distance through Disruption Morphology | 3.6 | 51 | Citations (PDF) |
| 73 | Theory of Star Formation | 22.4 | 2,207 | Citations (PDF) |
| 74 | Bondi‐Hoyle Accretion in a Turbulent Medium | 3.6 | 86 | Citations (PDF) |
| 75 | A Galactic Origin for the Local Ionized X‐Ray Absorbers | 3.6 | 79 | Citations (PDF) |
| 76 | Equilibrium Star Cluster Formation | 3.6 | 202 | Citations (PDF) |
| 77 | The Heavy‐Ion Approximation for Ambipolar Diffusion Calculations for Weakly Ionized Plasmas | 3.6 | 40 | Citations (PDF) |
| 78 | On the Hydrodynamic Interaction of Shock Waves with Interstellar Clouds. II. The Effect of Smooth Cloud Boundaries on Cloud Destruction and Cloud Turbulence | 4.9 | 137 | Citations (PDF) |
| 79 | The Global Evolution of Giant Molecular Clouds. I. Model Formulation and Quasi‐Equilibrium Behavior | 3.6 | 174 | Citations (PDF) |
| 80 | A General Theory of Turbulence‐regulated Star Formation, from Spirals to Ultraluminous Infrared Galaxies | 3.6 | 923 | Citations (PDF) |
| 81 | How Protostellar Outflows Help Massive Stars Form | 3.6 | 121 | Citations (PDF) |
| 82 | Cosmic‐Ray Acceleration at the Forward Shock in Tycho’s Supernova Remnant: Evidence fromChandraX‐Ray Observations | 3.6 | 283 | Citations (PDF) |
| 83 | Bondi Accretion in the Presence of Vorticity | 3.6 | 72 | Citations (PDF) |
| 84 | The formation of stars by gravitational collapse rather than competitive accretion | 31.3 | 136 | Citations (PDF) |
| 85 | An unsplit, cell-centered Godunov method for ideal MHD | 2.9 | 54 | Citations (PDF) |
| 86 | Far‐Infrared SEDs of Embedded Protostars and Dusty Galaxies. I. Theory for Spherical Sources | 3.6 | 41 | Citations (PDF) |
| 87 | Embedding Lagrangian Sink Particles in Eulerian Grids | 3.6 | 237 | Citations (PDF) |
| 88 | The Formation of the First Stars. I. Mass Infall Rates, Accretion Disk Structure, and Protostellar Evolution | 3.6 | 192 | Citations (PDF) |
| 89 | Neutral Atomic Phases of the Interstellar Medium in the Galaxy | 3.6 | 1,012 | Citations (PDF) |
| 90 | Time Dependence of the Ultraviolet Radiation Field in the Local Interstellar Medium | 3.6 | 99 | Citations (PDF) |
| 91 | The Formation of Massive Stars from Turbulent Cores | 3.6 | 920 | Citations (PDF) |
| 92 | Atomic Hydrogen Gas in Dark Matter Minihalos and the Compact High‐Velocity Clouds | 4.9 | 128 | Citations (PDF) |
| 93 | Massive star formation in 100,000 years from turbulent and pressurized molecular clouds | 31.3 | 333 | Citations (PDF) |
| 94 | Photoionization of Galactic Halo Gas by Old Supernova Remnants | 3.6 | 34 | Citations (PDF) |
| 95 | Doppler Shift Asymmetry in High‐Velocity Maser Emission from Shocks in Circumnuclear Disks | 3.6 | 58 | Citations (PDF) |
| 96 | The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-gravitational Hydrodynamics | 3.6 | 834 | Citations (PDF) |
| 97 | The Galactic Distribution of OB Associations in Molecular Clouds | 3.6 | 323 | Citations (PDF) |
| 98 | The Luminosity Function of OB Associations in the Galaxy | 3.6 | 295 | Citations (PDF) |
| 99 | Hydromagnetic Accretion Shocks around Low-Mass Protostars | 3.6 | 70 | Citations (PDF) |
| 100 | Equiparatition of energy for turbulent astrophysical fluids: Accounting for the unseen energy in molecular clouds | 3.6 | 53 | Citations (PDF) |
| 101 | Alfven Waves in Interstellar Gasdynamics | 3.6 | 95 | Citations (PDF) |
| 102 | The Multiphase Structure of the Galactic Halo: High-Velocity Clouds in a Hot Corona | 3.6 | 185 | Citations (PDF) |
| 103 | Shock interactions with magnetized interstellar clouds. 1: Steady shocks hitting nonradiative clouds | 3.6 | 158 | Citations (PDF) |
| 104 | Dynamics of Wind Bubbles and Superbubbles. II. Analytic Theory | 3.6 | 127 | Citations (PDF) |
| 105 | Pressure-confined clumps in magnetized molecular clouds | 3.6 | 766 | Citations (PDF) |
| 106 | On the virial theorem for turbulent molecular clouds | 3.6 | 134 | Citations (PDF) |
| 107 | Theoretical Astrophysics | 0.2 | 1 | Citations (PDF) |
| 108 | The photoevaporation of interstellar clouds. II - Equilibrium cometary clouds | 3.6 | 231 | Citations (PDF) |
| 109 | Photoionization-regulated star formation and the structure of molecular clouds | 3.6 | 484 | Citations (PDF) |
| 110 | Astrophysical blastwaves | 29.4 | 392 | Citations (PDF) |
| 111 | The injection of energy into the interstellar medium by stars (invited review) | 1.2 | 13 | Citations (PDF) |
| 112 | Trail of the Crab progenitor star | 31.3 | 13 | Citations (PDF) |
| 113 | Scaling of Ablative Laser-Fusion Implosions | 5.8 | 35 | Citations (PDF) |
| 114 | Effects of Flow on Density Profiles in Laser-Irradiated Plasmas | 5.8 | 64 | Citations (PDF) |
| 115 | X-Ray Emission from an Inward-Propagating Shock in Young Supernova Remnants | 3.6 | 131 | Citations (PDF) |
| 116 | Simulation of Counterstreaming Plasmas with Application to Collisionless Electrostatic Shocks | 5.8 | 25 | Citations (PDF) |
