All Stories

  1. An Origin of Radially Aligned Filaments in Hub-filament Systems
  2. Modeling of Collisional Outcomes Based on Impact Simulations of Mars-sized Bodies
  3. Fragmenting Filaments and Evolving Cores—Insights from Dust Polarization Study of a Filament in Northern Orion B
  4. The Dynamical Interaction between Low-mass Planets and Dust Coagulation
  5. Evolution of magnetized hub-filament systems
  6. Growth of Massive Molecular Cloud Filament by Accretion Flows. II. New Mechanism to Support a Supercritical Filament Against Radial Collapse
  7. Analytical and numerical linear analyses of convection revisited
  8. Erratum: “Two-dimensional Study of the Propagation of Planetary Wake and the Indication of Gap Opening in an Inviscid Protoplanetary Disk” (2010, ApJ, 724, 448)
  9. MHD Simulation in Galactic Center Region with Radiative Cooling and Heating
  10. Evolution of the Angular Momentum of Molecular Cloud Cores in Magnetized Molecular Filaments
  11. Growth of Massive Molecular Cloud Filament by Accretion Flows. I. Slow-shock Instability versus Ambipolar Diffusion
  12. Giant Impact Events for Protoplanets: Energetics of Atmospheric Erosion by Head-on Collision
  13. On Secular Gravitational Instability in Vertically Stratified Disks
  14. Triple Spiral Arms of a Triple Protostar System Imaged in Molecular Lines
  15. An Origin of Narrow Extended Structure in the Interstellar Medium: An Interstellar Contrail Created by a Fast-moving Massive Object
  16. Planetesimal Formation by the Gravitational Instability of Dust Ring Structures
  17. JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334
  18. Evolution of the Angular Momentum of Molecular Cloud Cores Formed from Filament Fragmentation
  19. Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. II. Dust-ring Formation Mediated by Backreaction and Fragmentation
  20. Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. I. First Numerical Study of Accelerated Dust Growth and Dust Concentration at Outer Radii
  21. Effects of Magnetic Field Orientations in Dense Cores on Gas Kinematics in Protostellar Envelopes
  22. The Effects of Cosmic-Ray Diffusion and Radiative Cooling on the Galactic Wind of the Milky Way
  23. Coagulation Instability in Protoplanetary Disks: A Novel Mechanism Connecting Collisional Growth and Hydrodynamical Clumping of Dust Particles
  24. Erratum: Dispersal of protoplanetary discs by the combination of magnetically driven and photoevaporative winds
  25. “Ashfall” Induced by Molecular Outflow in Protostar Evolution
  26. Classification of Filament Formation Mechanisms in Magnetized Molecular Clouds
  27. Conditions for Justifying Single-fluid Approximation for Charged and Neutral Dust Fluids and a Smoothed Particle Magnetohydrodynamics Method for Dust–Gas Mixture
  28. FAUST. II. Discovery of a Secondary Outflow in IRAS 15398−3359: Variability in Outflow Direction during the Earliest Stage of Star Formation?
  29. Bimodal Behavior and Convergence Requirement in Macroscopic Properties of the Multiphase Interstellar Medium Formed by Atomic Converging Flows
  30. 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
  31. Secular Gravitational Instability of Drifting Dust in Protoplanetary Disks: Formation of Dusty Rings without Significant Gas Substructures
  32. Early Evolution of Disk, Outflow, and Magnetic Field of Young Stellar Objects: Impact of Dust Model
  33. High-resolution simulations of catastrophic disruptions: Resultant shape distributions
  34. Dispersal of protoplanetary discs by the combination of magnetically driven and photoevaporative winds
  35. Revised Description of Dust Diffusion and a New Instability Creating Multiple Rings in Protoplanetary Disks
  36. Discovery of Shocked Molecular Clouds Associated with the Shell-type Supernova Remnant RX J0046.5−7308 in the Small Magellanic Cloud
  37. An Origin for the Angular Momentum of Molecular Cloud Cores: A Prediction from Filament Fragmentation
  38. Collisional elongation: Possible origin of extremely elongated shape of 1I/‘Oumuamua
  39. Constraints on the formation of brown dwarfs by turbulent compression
  40. The Generalized Nonlinear Ohm's Law: How a Strong Electric Field Influences Nonideal MHD Effects in Dusty Protoplanetary Disks
  41. A centrally concentrated sub-solar-mass starless core in the Taurus L1495 filamentary complex
  42. The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-forming Region
  43. The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C
  44. JCMT BISTRO Survey: Magnetic Fields within the Hub-filament Structure in IC 5146
  45. Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma-Rays and Interstellar Atomic Protons
  46. 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
  47. The Role of Magnetic Field in Molecular Cloud Formation and Evolution
  48. Erratum: “An Origin of Multiple Ring Structure and Hidden Planets in HL Tau: A Unified Picture by Secular Gravitational Instability” (2016, AJ, 152, 184)
  49. ALMA CO Observations of Supernova Remnant N63A in the Large Magellanic Cloud: Discovery of Dense Molecular Clouds Embedded within Shock-ionized and Photoionized Nebulae
  50. The Early Stage of Molecular Cloud Formation by Compression of Two-phase Atomic Gases
  51. Erratum: “Two-component Secular Gravitational Instability in a Protoplanetary Disk: A Possible Mechanism for Creating Ring-like Structures” (2014, ApJ, 794, 55)
  52. The Exchange of Mass and Angular Momentum in the Impact Event of Ice Giant Planets: Implications for the Origin of Uranus
  53. Radiation-hydrodynamic Simulations of Spherical Protostellar Collapse for Very Low-mass Objects
  54. Toward understanding the origin of asteroid geometries
  55. Does Misalignment between Magnetic Field and Angular Momentum Enhance or Suppress Circumstellar Disk Formation?
  56. ALMA Reveals a Misaligned Inner Gas Disk inside the Large Cavity of a Transitional Disk
  57. Properties of an accretion disc with a power-law stress–pressure relationship
  58. Molecular filament formation and filament–cloud interaction: Hints from Nobeyama 45 m telescope observations
  59. ALMA Observations of Supernova Remnant N49 in the LMC. I. Discovery of CO Clumps Associated with X-Ray and Radio Continuum Shells
  60. Numerical Simulations of Catastrophic Impacts Resolving Shapes of Remnants
  61. The impact of non-ideal effects on the circumstellar disk evolution and their observational signatures
  62. The role of magnetic field in the formation and evolution of filamentary molecular clouds
  63. Warm CO Gas Generated by Possible Turbulent Shocks in a Low-mass Star-forming Dense Core in Taurus
  64. Magnetic Fields toward Ophiuchus-B Derived from SCUBA-2 Polarization Measurements
  65. A Fast and Accurate Method of Radiation Hydrodynamics Calculation in Spherical Symmetry
  66. A First Look at BISTRO Observations of the ρ Oph-A core
  67. Differences in the Gas and Dust Distribution in the Transitional Disk of a Sun-like Young Star, PDS 70
  68. Star formation induced by cloud–cloud collisions and galactic giant molecular cloud evolution
  69. The diverse lives of massive protoplanets in self-gravitating discs
  70. 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)
  71. Non-linear development of secular gravitational instability in protoplanetary disks
  72. The impact of the Hall effect during cloud core collapse: Implications for circumstellar disk evolution
  73. 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
  74. Electron Heating and Saturation of Self-regulating Magnetorotational Instability in Protoplanetary Disks
  75. How Do Stars Gain Their Mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star-forming Regions
  76. The formation of massive molecular filaments and massive stars triggered by a magnetohydrodynamic shock wave
  77. Erratum: A revised condition for self-gravitational fragmentation of protoplanetary discs
  78. First Results from BISTRO: A SCUBA-2 Polarimeter Survey of the Gould Belt
  79. Theoretical Models of Protostellar Binary and Multiple Systems with AMR Simulations
  80. Faint warm debris disks around nearby bright stars explored by AKARI and IRSF
  81. Planet Formation in AB Aurigae: Imaging of the Inner Gaseous Spirals Observed inside the Dust Cavity
  82. Circumstellar Disks and Outflows in Turbulent Molecular Cloud Cores: Possible Formation Mechanism for Misaligned Systems
  83. DEBRIS DISKS AND THE ZODIACAL LIGHT EXPLORED BY THE AKARI MID-INFRARED ALL-SKY SURVEY
  84. An extension of Godunov SPH II: Application to elastic dynamics
  85. Evolutionary Description of Giant Molecular Cloud Mass Functions on Galactic Disks
  86. FORMATION OF H i CLOUDS IN SHOCK-COMPRESSED INTERSTELLAR MEDIUM: PHYSICAL ORIGIN OF ANGULAR CORRELATION BETWEEN FILAMENTARY STRUCTURE AND MAGNETIC FIELD
  87. AN ORIGIN OF MULTIPLE RING STRUCTURE AND HIDDEN PLANETS IN HL TAU: A UNIFIED PICTURE BY SECULAR GRAVITATIONAL INSTABILITY
  88. The origin of rotation profiles in star-forming clouds
  89. Conditions for circumstellar disc formation – II. Effects of initial cloud stability and mass accretion rate
  90. REVEALING A DETAILED MASS DISTRIBUTION OF A HIGH-DENSITY CORE MC27/L1521F IN TAURUS WITH ALMA
  91. Time Evolution of the Giant Molecular Cloud Mass Functions across Galactic Disks
  92. STOCHASTIC PARTICLE ACCELERATION IN TURBULENCE GENERATED BY MAGNETOROTATIONAL INSTABILITY
  93. Atmospheric Electrification in Dusty, Reactive Gases in the Solar System and Beyond
  94. DUST DYNAMICS IN PROTOPLANETARY DISK WINDS DRIVEN BY MAGNETOROTATIONAL TURBULENCE: A MECHANISM FOR FLOATING DUST GRAINS WITH CHARACTERISTIC SIZES
  95. A revised condition for self-gravitational fragmentation of protoplanetary discs
  96. An extension of Godunov SPH: Application to negative pressure media
  97. Diffusion of cosmic rays in a multiphase interstellar medium swept-up by a supernova remnant blast wave
  98. DEVELOPMENT OF A METHOD FOR THE OBSERVATION OF LIGHTNING IN PROTOPLANETARY DISKS USING ION LINES
  99. ON THE RADIUS ANOMALY OF HOT JUPITERS: REEXAMINATION OF THE POSSIBILITY AND IMPACT OF LAYERED CONVECTION
  100. Significant gas-to-dust ratio asymmetry and variation in the disk of HD 142527 and the indication of gas depletion
  101. BIMODALITY OF CIRCUMSTELLAR DISK EVOLUTION INDUCED BY THE HALL CURRENT
  102. ATMOSPHERIC ESCAPE BY MAGNETICALLY DRIVEN WIND FROM GASEOUS PLANETS. II. EFFECTS OF MAGNETIC DIFFUSION
  103. ALMA Observations of a High-density Core in Taurus: Dynamical Gas Interaction at the Possible Site of a Multiple Star Formation
  104. Star Formation
  105. The formation and destruction of molecular clouds and galactic star formation
  106. EXTREMELY BRIGHT SUBMILLIMETER GALAXIES BEYOND THE LUPUS-I STAR-FORMING REGION
  107. Effects of Ohmic and ambipolar diffusion on formation and evolution of first cores, protostars, and circumstellar discs
  108. Formation of terrestrial planets in disks evolving via disk winds and implications for the origin of the solar system’s terrestrial planets
  109. An origin of arc structures deeply embedded in dense molecular cloud cores
  110. THE NONLINEAR OHM'S LAW: PLASMA HEATING BY STRONG ELECTRIC FIELDS AND ITS EFFECTS ON THE IONIZATION BALANCE IN PROTOPLANETARY DISKS
  111. A DETAILED STUDY OF NON-THERMAL X-RAY PROPERTIES AND INTERSTELLAR GAS TOWARD THE γ-RAY SUPERNOVA REMNANT RX J1713.7–3946
  112. Low-Mass Star Formation: From Molecular Cloud Cores to Protostars and Protoplanetary Disks
  113. The Evolution of Giant Molecular Cloud Mass Function due to Cloud-Cloud Collisions
  114. Effects of radiative transfer on the structure of self-gravitating discs, their fragmentation and the evolution of the fragments
  115. A STATISTICAL ANALYSIS OF SEEDS AND OTHER HIGH-CONTRAST EXOPLANET SURVEYS: MASSIVE PLANETS OR LOW-MASS BROWN DWARFS?
  116. TWO-COMPONENT SECULAR GRAVITATIONAL INSTABILITY IN A PROTOPLANETARY DISK: A POSSIBLE MECHANISM FOR CREATING RING-LIKE STRUCTURES
  117. ATMOSPHERIC ESCAPE BY MAGNETICALLY DRIVEN WIND FROM GASEOUS PLANETS
  118. ALMA OBSERVATIONS OF A HIGH-DENSITY CORE IN TAURUS: DYNAMICAL GAS INTERACTION AT THE POSSIBLE SITE OF A MULTIPLE STAR FORMATION
  119. N-BODY SIMULATIONS OF TERRESTRIAL PLANET FORMATION UNDER THE INFLUENCE OF A HOT JUPITER
  120. ON THE VIABILITY OF THE MAGNETOROTATIONAL INSTABILITY IN CIRCUMPLANETARY DISKS
  121. MAGNETOHYDRODYNAMIC SIMULATIONS OF GLOBAL ACCRETION DISKS WITH VERTICAL MAGNETIC FIELDS
  122. SELF-SUSTAINED TURBULENCE WITHOUT DYNAMICAL FORCING: A TWO-DIMENSIONAL STUDY OF A BISTABLE INTERSTELLAR MEDIUM
  123. Dynamical Model Based on Hydrodynamics for Relativistic Heavy-Ion Collisions
  124. Conditions for circumstellar disc formation: effects of initial cloud configuration and sink treatment
  125. A new scheme of causal viscous hydrodynamics for relativistic heavy-ion collisions: A Riemann solver for quark–gluon plasma
  126. From Filamentary Networks to Dense Cores in Molecular Clouds: Toward a New Paradigm for Star Formation
  127. Magnetohydrodynamics with Time-Dependent Ionization Degree in Protoplanetary Disks with Grain Evolution
  128. The Effect of Mass Accretion for Formation and Thermal Evolution of Circumstellar Disks
  129. The Formation and Early Evolution of Protostars and Protoplanetary Disks
  130. Local Enhancement of the Surface Density in the Protoplanetary Ring Surrounding HD 142527
  131. CROWDING-OUT OF GIANTS BY DWARFS: AN ORIGIN FOR THE LACK OF COMPANION PLANETS IN HOT JUPITER SYSTEMS
  132. 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
  133. Formation, orbital and thermal evolution, and survival of planetary-mass clumps in the early phase of circumstellar disc evolution
  134. An explicit scheme for ohmic dissipation with smoothed particle magnetohydrodynamics
  135. ERRATUM: “INTERDEPENDENCE OF ELECTRIC DISCHARGE AND THE MAGNETOROTATIONAL INSTABILITY IN PROTOPLANETARY DISKS” (2012, ApJ, 760, 56)
  136. A SEMI-ANALYTICAL DESCRIPTION FOR THE FORMATION AND GRAVITATIONAL EVOLUTION OF PROTOPLANETARY DISKS
  137. High-Resolution Near-Infrared Polarimetry of a Circumstellar Disk around UX Tau A
  138. INTERDEPENDENCE OF ELECTRIC DISCHARGE AND MAGNETOROTATIONAL INSTABILITY IN PROTOPLANETARY DISKS
  139. FORMATION OF TURBULENT AND MAGNETIZED MOLECULAR CLOUDS VIA ACCRETION FLOWS OF H I CLOUDS
  140. Stability properties of phase transition layers in the diffuse ISM revisited
  141. ENHANCED DISSIPATION RATE OF MAGNETIC FIELD IN STRIPED PULSAR WINDS BY THE EFFECT OF TURBULENCE
  142. TOWARD UNDERSTANDING THE ORIGIN OF TURBULENCE IN MOLECULAR CLOUDS: SMALL-SCALE STRUCTURES AS UNITS OF DYNAMICAL MULTI-PHASE INTERSTELLAR MEDIUM
  143. Structure of dynamical condensation fronts in the interstellar medium
  144. THE MISSING CAVITIES IN THE SEEDS POLARIZED SCATTERED LIGHT IMAGES OF TRANSITIONAL PROTOPLANETARY DISKS: A GENERIC DISK MODEL
  145. DISCOVERY OF SMALL-SCALE SPIRAL STRUCTURES IN THE DISK OF SAO 206462 (HD 135344B): IMPLICATIONS FOR THE PHYSICAL STATE OF THE DISK FROM SPIRAL DENSITY WAVE THEORY
  146. 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
  147. SECULAR GRAVITATIONAL INSTABILITY OF A DUST LAYER IN SHEAR TURBULENCE
  148. An efficient dissipation mechanism of magnetic field by turbulence
  149. Cosmic-ray acceleration at young and middle-aged supernova remnants interacting with interstellar clouds
  150. Present-day star formation: From molecular cloud cores to protostars and protoplanetary disks
  151. TOWARD UNDERSTANDING THE COSMIC-RAY ACCELERATION AT YOUNG SUPERNOVA REMNANTS INTERACTING WITH INTERSTELLAR CLOUDS: POSSIBLE APPLICATIONS TO RX J1713.7–3946
  152. A FAST AND ACCURATE CALCULATION SCHEME FOR IONIZATION DEGREES IN PROTOPLANETARY AND CIRCUMPLANETARY DISKS WITH CHARGED DUST GRAINS
  153. Smoothed particle magnetohydrodynamics with a Riemann solver and the method of characteristics
  154. A fast numerical scheme for causal relativistic hydrodynamics with dissipation
  155. Effect of Magnetic Braking on Circumstellar Disk Formation in a Strongly Magnetized Cloud
  156. GRAVITATIONAL FRAGMENTATION OF EXPANDING SHELLS. I. LINEAR ANALYSIS
  157. GRAVITATIONAL FRAGMENTATION OF EXPANDING SHELLS. II. THREE-DIMENSIONAL SIMULATIONS
  158. DIRECT IMAGING OF FINE STRUCTURES IN GIANT PLANET-FORMING REGIONS OF THE PROTOPLANETARY DISK AROUND AB AURIGAE
  159. RECURRENT PLANET FORMATION AND INTERMITTENT PROTOSTELLAR OUTFLOWS INDUCED BY EPISODIC MASS ACCRETION
  160. FORMATION PROCESS OF THE CIRCUMSTELLAR DISK: LONG-TERM SIMULATIONS IN THE MAIN ACCRETION PHASE OF STAR FORMATION
  161. TWO-DIMENSIONAL STUDY OF THE PROPAGATION OF PLANETARY WAKE AND THE INDICATION OF GAP OPENING IN AN INVISCID PROTOPLANETARY DISK
  162. The relativistic kinetic dispersion relation: Comparison of the relativistic Bhatnagar–Gross–Krook model and Grad’s 14-moment expansion
  163. STAR-FORMING DENSE CLOUD CORES IN THE TeV GAMMA-RAY SNR RX J1713.7–3946
  164. TWO-STEP ACCELERATION MODEL OF COSMIC RAYS AT MIDDLE-AGED SUPERNOVA REMNANTS: UNIVERSALITY IN SECONDARY SHOCKS
  165. High-contrast polarimetric imaging of the protoplanetary disk around AB Aurigae
  166. N-BODY SIMULATION OF PLANETESIMAL FORMATION THROUGH GRAVITATIONAL INSTABILITY OF A DUST LAYER IN LAMINAR GAS DISK
  167. PROTOPLANETARY DISK WINDS VIA MAGNETOROTATIONAL INSTABILITY: FORMATION OF AN INNER HOLE AND A CRUCIAL ASSIST FOR PLANET FORMATION
  168. EMERGENCE OF PROTOPLANETARY DISKS AND SUCCESSIVE FORMATION OF GASEOUS PLANETS BY GRAVITATIONAL INSTABILITY
  169. Analysis of the Relaxation Process Using Nonrelativistic Kinetic Equation
  170. Kelvin-Helmholtz instabilities with Godunov smoothed particle hydrodynamics
  171. Gas accretion onto a protoplanet and formation of a gas giant planet
  172. Multi-Phase Dynamics of Magnetized Interstellar Medium
  173. Binary formation with different metallicities: dependence on initial conditions
  174. THE CIRCUMBINARY OUTFLOW: A PROTOSTELLAR OUTFLOW DRIVEN BY A CIRCUMBINARY DISK
  175. TWO-FLUID MAGNETOHYDRODYNAMICS SIMULATIONS OF CONVERGING H I FLOWS IN THE INTERSTELLAR MEDIUM. II. ARE MOLECULAR CLOUDS GENERATED DIRECTLY FROM A WARM NEUTRAL MEDIUM?
  176. N-BODY SIMULATION OF PLANETESIMAL FORMATION THROUGH GRAVITATIONAL INSTABILITY AND COAGULATION. II. ACCRETION MODEL
  177. EMISSION FROM A YOUNG PROTOSTELLAR OBJECT. I. SIGNATURES OF YOUNG EMBEDDED OUTFLOWS
  178. LOCAL LINEAR ANALYSIS OF INTERACTION BETWEEN A PLANET AND VISCOUS DISK AND AN IMPLICATION ON TYPE I PLANETARY MIGRATION
  179. FIRST DIRECT SIMULATION OF BROWN DWARF FORMATION IN A COMPACT CLOUD CORE
  180. ORBITAL EVOLUTION OF A PARTICLE INTERACTING WITH A SINGLE PLANET IN A PROTOPLANETARY DISK
  181. TURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM
  182. SUPERNOVA PROPAGATION AND CLOUD ENRICHMENT: A NEW MODEL FOR THE ORIGIN OF 60 Fe IN THE EARLY SOLAR SYSTEM
  183. DISK WINDS DRIVEN BY MAGNETOROTATIONAL INSTABILITY AND DISPERSAL OF PROTOPLANETARY DISKS
  184. A Hybrid Scenario for Planet Formation
  185. Protoplanetary Disk Formation in Molecular Cloud Cores
  186. Dispersal of Protoplanetary Disks by MHD Turbulence-Driven Disk Winds
  187. Orbital Evolution of Particles Embedded in a Protoplanetary Disk and the Possibility of Observing Low-mass Planets in a Protoplanetary∕Debris Disk
  188. Protostellar Jet and Outflow in the Collapsing Cloud Core
  189. DIRECT SIMULATIONS OF PARTICLE ACCELERATION IN A FLUCTUATING ELECTROMAGNETIC FIELD ACROSS A SHOCK
  190. Two‐Fluid Magnetohydrodynamic Simulations of Converging HiFlows in the Interstellar Medium. I. Methodology and Basic Results
  191. Angular Momentum Accretion onto a Gas Giant Planet
  192. Magnetohydrodynamics of Population III Star Formation
  193. The Effect of Poloidal Magnetic Field on Type I Planetary Migration: Significance of Magnetic Resonance
  194. The space infrared telescope for cosmology and astrophysics: SPICA A joint mission between JAXA and ESA
  195. Conditions for the Formation of First‐Star Binaries
  196. Formation Scenario for Wide and Close Binary Systems
  197. High‐ and Low‐Velocity Magnetized Outflows in the Star Formation Process in a Gravitationally Collapsing Cloud
  198. Evaporation of Tiny HI Clouds: Possible Probes of Physical State of the Galactic Gas Disk
  199. Magnetic Fields and Rotations of Protostars
  200. The effect of poloidal magnetic field on type I planetary migration
  201. Dynamical Formation of Dark Molecular Hydrogen Clouds around Diffuse HiiRegions
  202. Evolutionary Conditions in Dissipative MHD Systems Revisited
  203. Synthetic Observations of Carbon Lines of Turbulent Flows in the Diffuse Multiphase Interstellar Medium
  204. The Role of Ambipolar Diffusion in the Formation Process of Moderately Magnetized Diffuse Clouds
  205. N‐Body Simulation of Planetesimal Formation through Gravitational Instability of a Dust Layer
  206. Structure and Stability of Phase Transition Layers in the Interstellar Medium
  207. How Long Can Tiny H i Clouds Survive?
  208. Outflows Driven by Giant Protoplanets
  209. Dynamical Expansion of Ionization and Dissociation Front around a Massive Star: A Starburst Mechanism
  210. Can Warm Neutral Medium Survive inside Molecular Clouds?
  211. Second Core Formation and High-Speed Jets: Resistive Magnetohydrodynamic Nested Grid Simulations
  212. Dust evolution in photoevaporating protoplanetary disks
  213. Synthetic observations of turbulent flows in diffuse multiphase interstellar medium
  214. The First Jets in the Universe: Protostellar Jets from the First Stars
  215. Dynamical Expansion of Ionization and Dissociation Front around a Massive Star. II. On the Generality of Triggered Star Formation
  216. 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])
  217. Solar winds driven by nonlinear low‐frequency Alfvén waves from the photosphere: Parametric study for fast/slow winds and disappearance of solar winds
  218. 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
  219. 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
  220. Self-sustained Ionization and Vanishing Dead Zones in Protoplanetary Disks
  221. Evaporation and condensation of H I clouds in thermally bistable interstellar media: semi-analytic description of isobaric dynamics of curved interfaces
  222. Dynamical Expansion of Ionization and Dissociation Fronts around a Massive Star. I. A Mode of Triggered Star Formation
  223. The Role of Thermal Instability in Interstellar Medium
  224. The Formation of Molecular Clouds
  225. Angular Momentum Transport by Magnetohydrodynamic Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability
  226. Detection of Shocked Molecular Gas by Full-Extent Mapping of the Supernova Remnant W44
  227. The Field Condition: A New Constraint on Spatial Resolution in Simulations of the Nonlinear Development of Thermal Instability
  228. Angular Momentum Transport by MHD Turbulence in Accretion Disks
  229. The Local Mass Conservation in SPH
  230. Reformulation of Smoothed Particle Hydrodynamics with Riemann Solver
  231. 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
  232. Shear Flows in Smoothed Particle Hydrodynamics
  233. Toward Understanding the Formation of Molecular Clouds
  234. Saturation and Thermalization of the Magnetorotational Instability: Recurrent Channel Flows and Reconnections
  235. The Mass Function of Molecular Cloud Cores
  236. Molecular Evolution in Collapsing Prestellar Cores
  237. An Origin of Supersonic Motions in Interstellar Clouds
  238. Development of Special Purpose Computer for Cosmic Hydrodynamics with SPH Method
  239. Filament Fragmentation
  240. Infall Signatures in Spectral Line Profiles of Protostellar Envelopes
  241. Molecular Cloud Formation in Shock‐compressed Layers
  242. Does Deuterium Enable the Formation of Primordial Brown Dwarfs?
  243. A Radiation Hydrodynamic Model for Protostellar Collapse. II. The Second Collapse and the Birth of a Protostar
  244. The First Light of the Subaru Telescope: A New Infrared Image of the Orion Nebula
  245. Criteria for Fragmentation of Rotating Isothermal Clouds. I. Semianalytic Approach
  246. Criteria for Fragmentation of Rotating Isothermal Clouds Revisited
  247. Does “τ≈1” Terminate the Isothermal Evolution of Collapsing Clouds?
  248. A Higher-Order Godunov Scheme for Non-Ideal Magnetohydrodynamics
  249. A Radiation Hydrodynamical Model for Protostellar Collapse
  250. Advanced Methods in Particle Hydrodynamics
  251. Development of a Special Purpose Computer for Cosmic Hydrodynamics Using the SPH Method
  252. Fragmentation and Core Formation in Dynamically Collapsing Rotating Clouds
  253. A Saturation Mechanism of Magnetorotational Instability Due to Ohmic Dissipation
  254. An Origin of Filamentary Structure in Molecular Clouds
  255. A Radiation Hydrodynamic Model for Protostellar Collapse. I. The First Collapse
  256. Isothermal compression curve of Al2SiO5 kyanite
  257. A Production Mechanism for Clusters of Dense Cores
  258. Star Formation: Theory and Modelling
  259. Self-similar solutions and the stability of collapsing isothermal filaments
  260. Does Deuterium Enable the Formation of Primordial Brown Dwarfs?