All Stories

  1. Growth of Massive Molecular Cloud Filament by Accretion Flows. I. Slow-shock Instability versus Ambipolar Diffusion
  2. Giant Impact Events for Protoplanets: Energetics of Atmospheric Erosion by Head-on Collision
  3. On Secular Gravitational Instability in Vertically Stratified Disks
  4. Triple Spiral Arms of a Triple Protostar System Imaged in Molecular Lines
  5. An Origin of Narrow Extended Structure in the Interstellar Medium: An Interstellar Contrail Created by a Fast-moving Massive Object
  6. Planetesimal Formation by the Gravitational Instability of Dust Ring Structures
  7. JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334
  8. Evolution of the Angular Momentum of Molecular Cloud Cores Formed from Filament Fragmentation
  9. Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. II. Dust-ring Formation Mediated by Backreaction and Fragmentation
  10. Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. I. First Numerical Study of Accelerated Dust Growth and Dust Concentration at Outer Radii
  11. Effects of Magnetic Field Orientations in Dense Cores on Gas Kinematics in Protostellar Envelopes
  12. The Effects of Cosmic-Ray Diffusion and Radiative Cooling on the Galactic Wind of the Milky Way
  13. Coagulation Instability in Protoplanetary Disks: A Novel Mechanism Connecting Collisional Growth and Hydrodynamical Clumping of Dust Particles
  14. Erratum: Dispersal of protoplanetary discs by the combination of magnetically driven and photoevaporative winds
  15. “Ashfall” Induced by Molecular Outflow in Protostar Evolution
  16. Classification of Filament Formation Mechanisms in Magnetized Molecular Clouds
  17. Conditions for Justifying Single-fluid Approximation for Charged and Neutral Dust Fluids and a Smoothed Particle Magnetohydrodynamics Method for Dust–Gas Mixture
  18. FAUST. II. Discovery of a Secondary Outflow in IRAS 15398−3359: Variability in Outflow Direction during the Earliest Stage of Star Formation?
  19. Bimodal Behavior and Convergence Requirement in Macroscopic Properties of the Multiphase Interstellar Medium Formed by Atomic Converging Flows
  20. ALMA CO Observations of the Gamma-Ray Supernova Remnant RX J1713.7–3946: Discovery of Shocked Molecular Cloudlets and Filaments at 0.01 pc Scales
  21. Secular Gravitational Instability of Drifting Dust in Protoplanetary Disks: Formation of Dusty Rings without Significant Gas Substructures
  22. Early Evolution of Disk, Outflow, and Magnetic Field of Young Stellar Objects: Impact of Dust Model
  23. High-resolution simulations of catastrophic disruptions: Resultant shape distributions
  24. Dispersal of protoplanetary discs by the combination of magnetically driven and photoevaporative winds
  25. Revised Description of Dust Diffusion and a New Instability Creating Multiple Rings in Protoplanetary Disks
  26. Discovery of Shocked Molecular Clouds Associated with the Shell-type Supernova Remnant RX J0046.5−7308 in the Small Magellanic Cloud
  27. An Origin for the Angular Momentum of Molecular Cloud Cores: A Prediction from Filament Fragmentation
  28. Collisional elongation: Possible origin of extremely elongated shape of 1I/‘Oumuamua
  29. Constraints on the formation of brown dwarfs by turbulent compression
  30. The Generalized Nonlinear Ohm's Law: How a Strong Electric Field Influences Nonideal MHD Effects in Dusty Protoplanetary Disks
  31. A centrally concentrated sub-solar-mass starless core in the Taurus L1495 filamentary complex
  32. The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-forming Region
  33. The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C
  34. JCMT BISTRO Survey: Magnetic Fields within the Hub-filament Structure in IC 5146
  35. Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma-Rays and Interstellar Atomic Protons
  36. FOREST Unbiased Galactic Plane Imaging Survey with the Nobeyama 45 m telescope (FUGIN). V. Dense gas mass fraction of molecular gas in the Galactic plane
  37. The Role of Magnetic Field in Molecular Cloud Formation and Evolution
  38. Erratum: “An Origin of Multiple Ring Structure and Hidden Planets in HL Tau: A Unified Picture by Secular Gravitational Instability” (2016, AJ, 152, 184)
  39. The Early Stage of Molecular Cloud Formation by Compression of Two-phase Atomic Gases
  40. Erratum: “Two-component Secular Gravitational Instability in a Protoplanetary Disk: A Possible Mechanism for Creating Ring-like Structures” (2014, ApJ, 794, 55)
  41. The Exchange of Mass and Angular Momentum in the Impact Event of Ice Giant Planets: Implications for the Origin of Uranus
  42. Radiation-hydrodynamic Simulations of Spherical Protostellar Collapse for Very Low-mass Objects
  43. Toward understanding the origin of asteroid geometries
  44. Does Misalignment between Magnetic Field and Angular Momentum Enhance or Suppress Circumstellar Disk Formation?
  45. ALMA Reveals a Misaligned Inner Gas Disk inside the Large Cavity of a Transitional Disk
  46. Properties of an accretion disc with a power-law stress–pressure relationship
  47. Molecular filament formation and filament–cloud interaction: Hints from Nobeyama 45 m telescope observations
  48. ALMA Observations of Supernova Remnant N49 in the LMC. I. Discovery of CO Clumps Associated with X-Ray and Radio Continuum Shells
  49. Numerical Simulations of Catastrophic Impacts Resolving Shapes of Remnants
  50. The impact of non-ideal effects on the circumstellar disk evolution and their observational signatures
  51. The role of magnetic field in the formation and evolution of filamentary molecular clouds
  52. Warm CO Gas Generated by Possible Turbulent Shocks in a Low-mass Star-forming Dense Core in Taurus
  53. Magnetic Fields toward Ophiuchus-B Derived from SCUBA-2 Polarization Measurements
  54. A Fast and Accurate Method of Radiation Hydrodynamics Calculation in Spherical Symmetry
  55. A First Look at BISTRO Observations of the ρ Oph-A core
  56. Differences in the Gas and Dust Distribution in the Transitional Disk of a Sun-like Young Star, PDS 70
  57. Star formation induced by cloud–cloud collisions and galactic giant molecular cloud evolution
  58. The diverse lives of massive protoplanets in self-gravitating discs
  59. Erratum: “Two-fluid Magnetohydrodynamics Simulations of Converging of H i Flows in the Interstellar Medium. II. Are Molecular Clouds Generated Directly from Warm Neutral Medium?” (2009, ApJ, 704, 161)
  60. Non-linear development of secular gravitational instability in protoplanetary disks
  61. The impact of the Hall effect during cloud core collapse: Implications for circumstellar disk evolution
  62. A Detached Protostellar Disk around a ∼0.2 M⊙ Protostar in a Possible Site of a Multiple Star Formation in a Dynamical Environment in Taurus
  63. Electron Heating and Saturation of Self-regulating Magnetorotational Instability in Protoplanetary Disks
  64. How Do Stars Gain Their Mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star-forming Regions
  65. The formation of massive molecular filaments and massive stars triggered by a magnetohydrodynamic shock wave
  66. Erratum: A revised condition for self-gravitational fragmentation of protoplanetary discs
  67. First Results from BISTRO: A SCUBA-2 Polarimeter Survey of the Gould Belt
  68. Theoretical Models of Protostellar Binary and Multiple Systems with AMR Simulations
  69. Faint warm debris disks around nearby bright stars explored by AKARI and IRSF
  70. Planet Formation in AB Aurigae: Imaging of the Inner Gaseous Spirals Observed inside the Dust Cavity
  71. Circumstellar Disks and Outflows in Turbulent Molecular Cloud Cores: Possible Formation Mechanism for Misaligned Systems
  72. An extension of Godunov SPH II: Application to elastic dynamics
  73. Evolutionary Description of Giant Molecular Cloud Mass Functions on Galactic Disks
  74. FORMATION OF H i CLOUDS IN SHOCK-COMPRESSED INTERSTELLAR MEDIUM: PHYSICAL ORIGIN OF ANGULAR CORRELATION BETWEEN FILAMENTARY STRUCTURE AND MAGNETIC FIELD
  75. AN ORIGIN OF MULTIPLE RING STRUCTURE AND HIDDEN PLANETS IN HL TAU: A UNIFIED PICTURE BY SECULAR GRAVITATIONAL INSTABILITY
  76. The origin of rotation profiles in star-forming clouds
  77. Conditions for circumstellar disc formation – II. Effects of initial cloud stability and mass accretion rate
  78. REVEALING A DETAILED MASS DISTRIBUTION OF A HIGH-DENSITY CORE MC27/L1521F IN TAURUS WITH ALMA
  79. Time Evolution of the Giant Molecular Cloud Mass Functions across Galactic Disks
  80. STOCHASTIC PARTICLE ACCELERATION IN TURBULENCE GENERATED BY MAGNETOROTATIONAL INSTABILITY
  81. Atmospheric Electrification in Dusty, Reactive Gases in the Solar System and Beyond
  82. DUST DYNAMICS IN PROTOPLANETARY DISK WINDS DRIVEN BY MAGNETOROTATIONAL TURBULENCE: A MECHANISM FOR FLOATING DUST GRAINS WITH CHARACTERISTIC SIZES
  83. A revised condition for self-gravitational fragmentation of protoplanetary discs
  84. An extension of Godunov SPH: Application to negative pressure media
  85. Diffusion of cosmic rays in a multiphase interstellar medium swept-up by a supernova remnant blast wave
  86. DEVELOPMENT OF A METHOD FOR THE OBSERVATION OF LIGHTNING IN PROTOPLANETARY DISKS USING ION LINES
  87. ON THE RADIUS ANOMALY OF HOT JUPITERS: REEXAMINATION OF THE POSSIBILITY AND IMPACT OF LAYERED CONVECTION
  88. Significant gas-to-dust ratio asymmetry and variation in the disk of HD 142527 and the indication of gas depletion
  89. BIMODALITY OF CIRCUMSTELLAR DISK EVOLUTION INDUCED BY THE HALL CURRENT
  90. ATMOSPHERIC ESCAPE BY MAGNETICALLY DRIVEN WIND FROM GASEOUS PLANETS. II. EFFECTS OF MAGNETIC DIFFUSION
  91. ALMA Observations of a High-density Core in Taurus: Dynamical Gas Interaction at the Possible Site of a Multiple Star Formation
  92. Star Formation
  93. The formation and destruction of molecular clouds and galactic star formation
  94. EXTREMELY BRIGHT SUBMILLIMETER GALAXIES BEYOND THE LUPUS-I STAR-FORMING REGION
  95. Effects of Ohmic and ambipolar diffusion on formation and evolution of first cores, protostars, and circumstellar discs
  96. Formation of terrestrial planets in disks evolving via disk winds and implications for the origin of the solar system’s terrestrial planets
  97. An origin of arc structures deeply embedded in dense molecular cloud cores
  98. THE NONLINEAR OHM'S LAW: PLASMA HEATING BY STRONG ELECTRIC FIELDS AND ITS EFFECTS ON THE IONIZATION BALANCE IN PROTOPLANETARY DISKS
  99. A DETAILED STUDY OF NON-THERMAL X-RAY PROPERTIES AND INTERSTELLAR GAS TOWARD THE γ-RAY SUPERNOVA REMNANT RX J1713.7–3946
  100. Low-Mass Star Formation: From Molecular Cloud Cores to Protostars and Protoplanetary Disks
  101. The Evolution of Giant Molecular Cloud Mass Function due to Cloud-Cloud Collisions
  102. Effects of radiative transfer on the structure of self-gravitating discs, their fragmentation and the evolution of the fragments
  103. A STATISTICAL ANALYSIS OF SEEDS AND OTHER HIGH-CONTRAST EXOPLANET SURVEYS: MASSIVE PLANETS OR LOW-MASS BROWN DWARFS?
  104. TWO-COMPONENT SECULAR GRAVITATIONAL INSTABILITY IN A PROTOPLANETARY DISK: A POSSIBLE MECHANISM FOR CREATING RING-LIKE STRUCTURES
  105. ATMOSPHERIC ESCAPE BY MAGNETICALLY DRIVEN WIND FROM GASEOUS PLANETS
  106. ALMA OBSERVATIONS OF A HIGH-DENSITY CORE IN TAURUS: DYNAMICAL GAS INTERACTION AT THE POSSIBLE SITE OF A MULTIPLE STAR FORMATION
  107. N-BODY SIMULATIONS OF TERRESTRIAL PLANET FORMATION UNDER THE INFLUENCE OF A HOT JUPITER
  108. ON THE VIABILITY OF THE MAGNETOROTATIONAL INSTABILITY IN CIRCUMPLANETARY DISKS
  109. MAGNETOHYDRODYNAMIC SIMULATIONS OF GLOBAL ACCRETION DISKS WITH VERTICAL MAGNETIC FIELDS
  110. SELF-SUSTAINED TURBULENCE WITHOUT DYNAMICAL FORCING: A TWO-DIMENSIONAL STUDY OF A BISTABLE INTERSTELLAR MEDIUM
  111. Dynamical Model Based on Hydrodynamics for Relativistic Heavy-Ion Collisions
  112. Conditions for circumstellar disc formation: effects of initial cloud configuration and sink treatment
  113. A new scheme of causal viscous hydrodynamics for relativistic heavy-ion collisions: A Riemann solver for quark–gluon plasma
  114. From Filamentary Networks to Dense Cores in Molecular Clouds: Toward a New Paradigm for Star Formation
  115. Magnetohydrodynamics with Time-Dependent Ionization Degree in Protoplanetary Disks with Grain Evolution
  116. CROWDING-OUT OF GIANTS BY DWARFS: AN ORIGIN FOR THE LACK OF COMPANION PLANETS IN HOT JUPITER SYSTEMS
  117. NON-THERMAL X-RAYS AND INTERSTELLAR GAS TOWARD THE γ-RAY SUPERNOVA REMNANT RX J1713.7–3946: EVIDENCE FOR X-RAY ENHANCEMENT AROUND CO AND H I CLUMPS
  118. Formation, orbital and thermal evolution, and survival of planetary-mass clumps in the early phase of circumstellar disc evolution
  119. ERRATUM: “INTERDEPENDENCE OF ELECTRIC DISCHARGE AND THE MAGNETOROTATIONAL INSTABILITY IN PROTOPLANETARY DISKS” (2012, ApJ, 760, 56)
  120. A SEMI-ANALYTICAL DESCRIPTION FOR THE FORMATION AND GRAVITATIONAL EVOLUTION OF PROTOPLANETARY DISKS
  121. High-Resolution Near-Infrared Polarimetry of a Circumstellar Disk around UX Tau A
  122. INTERDEPENDENCE OF ELECTRIC DISCHARGE AND MAGNETOROTATIONAL INSTABILITY IN PROTOPLANETARY DISKS
  123. FORMATION OF TURBULENT AND MAGNETIZED MOLECULAR CLOUDS VIA ACCRETION FLOWS OF H I CLOUDS
  124. Stability properties of phase transition layers in the diffuse ISM revisited
  125. ENHANCED DISSIPATION RATE OF MAGNETIC FIELD IN STRIPED PULSAR WINDS BY THE EFFECT OF TURBULENCE
  126. TOWARD UNDERSTANDING THE ORIGIN OF TURBULENCE IN MOLECULAR CLOUDS: SMALL-SCALE STRUCTURES AS UNITS OF DYNAMICAL MULTI-PHASE INTERSTELLAR MEDIUM
  127. THE MISSING CAVITIES IN THE SEEDS POLARIZED SCATTERED LIGHT IMAGES OF TRANSITIONAL PROTOPLANETARY DISKS: A GENERIC DISK MODEL
  128. A DETAILED STUDY OF THE MOLECULAR AND ATOMIC GAS TOWARD THE γ-RAY SUPERNOVA REMNANT RX J1713.7–3946: SPATIAL TeV γ-RAY AND INTERSTELLAR MEDIUM GAS CORRESPONDENCE
  129. SECULAR GRAVITATIONAL INSTABILITY OF A DUST LAYER IN SHEAR TURBULENCE
  130. An efficient dissipation mechanism of magnetic field by turbulence
  131. Present-day star formation: From molecular cloud cores to protostars and protoplanetary disks
  132. TOWARD UNDERSTANDING THE COSMIC-RAY ACCELERATION AT YOUNG SUPERNOVA REMNANTS INTERACTING WITH INTERSTELLAR CLOUDS: POSSIBLE APPLICATIONS TO RX J1713.7–3946
  133. Smoothed particle magnetohydrodynamics with a Riemann solver and the method of characteristics
  134. A fast numerical scheme for causal relativistic hydrodynamics with dissipation
  135. Effect of Magnetic Braking on Circumstellar Disk Formation in a Strongly Magnetized Cloud
  136. GRAVITATIONAL FRAGMENTATION OF EXPANDING SHELLS. II. THREE-DIMENSIONAL SIMULATIONS
  137. DIRECT IMAGING OF FINE STRUCTURES IN GIANT PLANET-FORMING REGIONS OF THE PROTOPLANETARY DISK AROUND AB AURIGAE
  138. RECURRENT PLANET FORMATION AND INTERMITTENT PROTOSTELLAR OUTFLOWS INDUCED BY EPISODIC MASS ACCRETION
  139. FORMATION PROCESS OF THE CIRCUMSTELLAR DISK: LONG-TERM SIMULATIONS IN THE MAIN ACCRETION PHASE OF STAR FORMATION
  140. The relativistic kinetic dispersion relation: Comparison of the relativistic Bhatnagar–Gross–Krook model and Grad’s 14-moment expansion
  141. TWO-STEP ACCELERATION MODEL OF COSMIC RAYS AT MIDDLE-AGED SUPERNOVA REMNANTS: UNIVERSALITY IN SECONDARY SHOCKS
  142. N-BODY SIMULATION OF PLANETESIMAL FORMATION THROUGH GRAVITATIONAL INSTABILITY OF A DUST LAYER IN LAMINAR GAS DISK
  143. Kelvin-Helmholtz instabilities with Godunov smoothed particle hydrodynamics
  144. Gas accretion onto a protoplanet and formation of a gas giant planet
  145. Multi-Phase Dynamics of Magnetized Interstellar Medium
  146. Binary formation with different metallicities: dependence on initial conditions
  147. THE CIRCUMBINARY OUTFLOW: A PROTOSTELLAR OUTFLOW DRIVEN BY A CIRCUMBINARY DISK
  148. TWO-FLUID MAGNETOHYDRODYNAMICS SIMULATIONS OF CONVERGING H I FLOWS IN THE INTERSTELLAR MEDIUM. II. ARE MOLECULAR CLOUDS GENERATED DIRECTLY FROM A WARM NEUTRAL MEDIUM?
  149. N-BODY SIMULATION OF PLANETESIMAL FORMATION THROUGH GRAVITATIONAL INSTABILITY AND COAGULATION. II. ACCRETION MODEL
  150. EMISSION FROM A YOUNG PROTOSTELLAR OBJECT. I. SIGNATURES OF YOUNG EMBEDDED OUTFLOWS
  151. LOCAL LINEAR ANALYSIS OF INTERACTION BETWEEN A PLANET AND VISCOUS DISK AND AN IMPLICATION ON TYPE I PLANETARY MIGRATION
  152. FIRST DIRECT SIMULATION OF BROWN DWARF FORMATION IN A COMPACT CLOUD CORE
  153. ORBITAL EVOLUTION OF A PARTICLE INTERACTING WITH A SINGLE PLANET IN A PROTOPLANETARY DISK
  154. TURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM
  155. SUPERNOVA PROPAGATION AND CLOUD ENRICHMENT: A NEW MODEL FOR THE ORIGIN OF 60 Fe IN THE EARLY SOLAR SYSTEM
  156. DISK WINDS DRIVEN BY MAGNETOROTATIONAL INSTABILITY AND DISPERSAL OF PROTOPLANETARY DISKS
  157. A Hybrid Scenario for Planet Formation
  158. Protoplanetary Disk Formation in Molecular Cloud Cores
  159. Dispersal of Protoplanetary Disks by MHD Turbulence-Driven Disk Winds
  160. Orbital Evolution of Particles Embedded in a Protoplanetary Disk and the Possibility of Observing Low-mass Planets in a Protoplanetary∕Debris Disk
  161. Protostellar Jet and Outflow in the Collapsing Cloud Core
  162. DIRECT SIMULATIONS OF PARTICLE ACCELERATION IN A FLUCTUATING ELECTROMAGNETIC FIELD ACROSS A SHOCK
  163. Two‐Fluid Magnetohydrodynamic Simulations of Converging HiFlows in the Interstellar Medium. I. Methodology and Basic Results
  164. Angular Momentum Accretion onto a Gas Giant Planet
  165. Magnetohydrodynamics of Population III Star Formation
  166. The Effect of Poloidal Magnetic Field on Type I Planetary Migration: Significance of Magnetic Resonance
  167. The space infrared telescope for cosmology and astrophysics: SPICA A joint mission between JAXA and ESA
  168. Conditions for the Formation of First‐Star Binaries
  169. Formation Scenario for Wide and Close Binary Systems
  170. High‐ and Low‐Velocity Magnetized Outflows in the Star Formation Process in a Gravitationally Collapsing Cloud
  171. Magnetic Fields and Rotations of Protostars
  172. The effect of poloidal magnetic field on type I planetary migration
  173. Dynamical Formation of Dark Molecular Hydrogen Clouds around Diffuse HiiRegions
  174. Synthetic Observations of Carbon Lines of Turbulent Flows in the Diffuse Multiphase Interstellar Medium
  175. N‐Body Simulation of Planetesimal Formation through Gravitational Instability of a Dust Layer
  176. Structure and Stability of Phase Transition Layers in the Interstellar Medium
  177. Outflows Driven by Giant Protoplanets
  178. Dynamical Expansion of Ionization and Dissociation Front around a Massive Star: A Starburst Mechanism
  179. Can Warm Neutral Medium Survive inside Molecular Clouds?
  180. Second Core Formation and High-Speed Jets: Resistive Magnetohydrodynamic Nested Grid Simulations
  181. Dust evolution in photoevaporating protoplanetary disks
  182. The First Jets in the Universe: Protostellar Jets from the First Stars
  183. Dynamical Expansion of Ionization and Dissociation Front around a Massive Star. II. On the Generality of Triggered Star Formation
  184. Erratum: "Making the Corona and the Fast Solar Wind: A Self-consistent Simulation for the Low-Frequency Alfvén Waves from Photosphere to 0.3 AU" ([URL ADDRESS="/cgi-bin/resolve?2005ApJ...632L..49S" STATUS="OKAY"]ApJ, 632, L49 [2005][/URL])
  185. Solar winds driven by nonlinear low‐frequency Alfvén waves from the photosphere: Parametric study for fast/slow winds and disappearance of solar winds
  186. A Two‐Fluid Analysis of the Kelvin‐Helmholtz Instability in the Dusty Layer of a Protoplanetary Disk: A Possible Path toward Planetesimal Formation through Gravitational Instability
  187. Making the Corona and the Fast Solar Wind: A Self-consistent Simulation for the Low-Frequency Alfvén Waves from the Photosphere to 0.3 AU
  188. Self-sustained Ionization and Vanishing Dead Zones in Protoplanetary Disks
  189. Evaporation and condensation of H I clouds in thermally bistable interstellar media: semi-analytic description of isobaric dynamics of curved interfaces
  190. Dynamical Expansion of Ionization and Dissociation Fronts around a Massive Star. I. A Mode of Triggered Star Formation
  191. The Role of Thermal Instability in Interstellar Medium
  192. The Formation of Molecular Clouds
  193. Angular Momentum Transport by Magnetohydrodynamic Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability
  194. Detection of Shocked Molecular Gas by Full-Extent Mapping of the Supernova Remnant W44
  195. The Field Condition: A New Constraint on Spatial Resolution in Simulations of the Nonlinear Development of Thermal Instability
  196. Angular Momentum Transport by MHD Turbulence in Accretion Disks
  197. Reformulation of Smoothed Particle Hydrodynamics with Riemann Solver
  198. An upper limit on the mass of a primordial star due to the formation of an H II region: the effect of ionizing radiation force
  199. Shear Flows in Smoothed Particle Hydrodynamics
  200. Saturation and Thermalization of the Magnetorotational Instability: Recurrent Channel Flows and Reconnections
  201. The Mass Function of Molecular Cloud Cores
  202. Molecular Evolution in Collapsing Prestellar Cores
  203. An Origin of Supersonic Motions in Interstellar Clouds
  204. Development of Special Purpose Computer for Cosmic Hydrodynamics with SPH Method
  205. Infall Signatures in Spectral Line Profiles of Protostellar Envelopes
  206. Molecular Cloud Formation in Shock‐compressed Layers
  207. Does Deuterium Enable the Formation of Primordial Brown Dwarfs?
  208. A Radiation Hydrodynamic Model for Protostellar Collapse. II. The Second Collapse and the Birth of a Protostar
  209. The First Light of the Subaru Telescope: A New Infrared Image of the Orion Nebula
  210. Criteria for Fragmentation of Rotating Isothermal Clouds. I. Semianalytic Approach
  211. Criteria for Fragmentation of Rotating Isothermal Clouds Revisited
  212. Does “τ≈1” Terminate the Isothermal Evolution of Collapsing Clouds?
  213. A Higher-Order Godunov Scheme for Non-Ideal Magnetohydrodynamics
  214. A Radiation Hydrodynamical Model for Protostellar Collapse
  215. Advanced Methods in Particle Hydrodynamics
  216. Development of a Special Purpose Computer for Cosmic Hydrodynamics Using the SPH Method
  217. Fragmentation and Core Formation in Dynamically Collapsing Rotating Clouds
  218. A Saturation Mechanism of Magnetorotational Instability Due to Ohmic Dissipation
  219. An Origin of Filamentary Structure in Molecular Clouds
  220. A Radiation Hydrodynamic Model for Protostellar Collapse. I. The First Collapse
  221. Isothermal compression curve of Al2SiO5 kyanite
  222. A Production Mechanism for Clusters of Dense Cores
  223. Star Formation: Theory and Modelling
  224. Self-similar solutions and the stability of collapsing isothermal filaments
  225. Does Deuterium Enable the Formation of Primordial Brown Dwarfs?