Comparing the statistics of interstellar turbulence in simulations and observations - Solenoidal versus compressive turbulence forcing
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[1] L. Hartmann,et al. The Birth of Molecular Clouds: Formation of Atomic Precursors in Colliding Flows , 2006, astro-ph/0605435.
[2] A. Goodman,et al. TMC-1C: An Accreting Starless Core , 2007, 0706.4115.
[3] C. Brunt,et al. Interstellar Turbulence. II. Energy Spectra of Molecular Regions in the Outer Galaxy , 2001, astro-ph/0110155.
[4] S. Boldyrev. Kolmogorov-Burgers Model for Star-forming Turbulence , 2001, astro-ph/0108300.
[5] M. Norman,et al. The Statistics of Supersonic Isothermal Turbulence , 2007, 0704.3851.
[6] France.,et al. Molecular Cloud Evolution. I. Molecular Cloud and Thin Cold Neutral Medium Sheet Formation , 2005, astro-ph/0509127.
[7] S. Glover,et al. Simulating the Formation of Molecular Clouds. I. Slow Formation by Gravitational Collapse from Static Initial Conditions , 2006, astro-ph/0605120.
[8] P. Woodward,et al. Synthesized spectra of turbulent clouds , 1994 .
[9] R. Jimenez,et al. Structure function scaling in compressible super-Alfvénic MHD turbulence. , 2003, Physical Review Letters.
[10] Richard M. Crutcher,et al. TESTING MAGNETIC STAR FORMATION THEORY , 2008, 0807.2862.
[11] R. Klessen,et al. Modelling CO formation in the turbulent interstellar medium , 2009, 0907.4081.
[12] A. Goodman,et al. THE “TRUE” COLUMN DENSITY DISTRIBUTION IN STAR-FORMING MOLECULAR CLOUDS , 2008, 0806.3441.
[13] Dissipative structures of diffuse molecular gas - III. Small-scale intermittency of intense velocity-shears , 2008, 0802.0758.
[14] Succi,et al. Extended self-similarity in turbulent flows. , 1993, Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics.
[15] E. Feigelson,et al. A Chandra Study of the Rosette Star-forming Complex. I. The Stellar Population and Structure of the Young Open Cluster NGC 2244 , 2007, 0711.2024.
[16] A. Azzalini. A class of distributions which includes the normal ones , 1985 .
[17] P. Hennebelle,et al. ANALYTICAL THEORY FOR THE INITIAL MASS FUNCTION. II. PROPERTIES OF THE FLOW , 2009, 0907.2765.
[18] I. Bohachevsky,et al. Finite difference method for numerical computation of discontinuous solutions of the equations of fluid dynamics , 1959 .
[19] R. Klessen,et al. MODELING COLLAPSE AND ACCRETION IN TURBULENT GAS CLOUDS: IMPLEMENTATION AND COMPARISON OF SINK PARTICLES IN AMR AND SPH , 2010, 1001.4456.
[20] J. Kainulainen. Probing the Evolution of Molecular Cloud Structure , 2010 .
[21] Richard B. Larson,et al. Numerical Calculations of the Dynamics of a Collapsing Proto-Star , 1969 .
[22] Paul R. Woodward,et al. Kolmogorov‐like spectra in decaying three‐dimensional supersonic flows , 1994 .
[23] K. Tassis. The star formation law in a multifractal ISM , 2007, 0709.1474.
[24] R. Klessen,et al. The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing , 2008, 0808.0605.
[25] Daniel J. Price,et al. A comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulence , 2010, 1004.1446.
[26] Javier Jiménez,et al. Geometry and clustering of intense structures in isotropic turbulence , 2004, Journal of Fluid Mechanics.
[27] Daniel J. Price,et al. A method for reconstructing the variance of a 3D physical field from 2D observations: application to turbulence in the interstellar medium , 2010, 1001.1046.
[28] Ralf Klessen,et al. Clump morphology and evolution in MHD simulations of molecular cloud formation , 2008, 0808.0986.
[29] R. Klessen,et al. Turbulent mixing in the interstellar medium: an application for Lagrangian tracer particles , 2008, 0805.0196.
[30] F. Anselmet,et al. High-order velocity structure functions in turbulent shear flows , 1984, Journal of Fluid Mechanics.
[31] A. Goodman,et al. CO Isotopologues in the Perseus Molecular Cloud Complex: the X-factor and Regional Variations , 2008, 0802.0708.
[32] S. Glover,et al. Simulating the Formation of Molecular Clouds. II. Rapid Formation from Turbulent Initial Conditions , 2006, astro-ph/0605121.
[33] C. Lada,et al. Sequential formation of subgroups in OB associations , 1977 .
[34] M. Penston. Dynamics of Self-Gravitating Gaseous Spheres—III: Analytical Results in the Free-fall of Isothermal Cases , 1969 .
[35] M. Lombardi,et al. The Nature of the Dense Core Population in the Pipe Nebula: Thermal Cores Under Pressure , 2007, 0709.1164.
[36] The COMPLETE Nature of the Warm Dust Shell in Perseus , 2006, astro-ph/0601692.
[37] Jongsoo Kim,et al. Core Mass Function: The Role of Gravity , 2008, 0801.2257.
[38] She,et al. Universal scaling laws in fully developed turbulence. , 1994, Physical review letters.
[39] E. Ostriker,et al. Dissipation in Compressible Magnetohydrodynamic Turbulence , 1998, astro-ph/9809357.
[40] D. Johnstone,et al. Dynamics of Dense Cores in the Perseus Molecular Cloud , 2007, 0707.2769.
[41] D. Breitschwerdt,et al. What Physical Processes Drive the Interstellar Medium in the Local Bubble? , 2009 .
[42] T. Passot,et al. Density probability distribution in one-dimensional polytropic gas dynamics , 1998, physics/9802019.
[43] I. A. Bonnell,et al. Modelling accretion in protobinary systems , 1995 .
[44] R. Grauer,et al. Local turbulence simulations for the multiphase ISM , 2008, 0901.4495.
[45] N. Haugen,et al. Bottleneck effect in three-dimensional turbulence simulations. , 2003, Physical review. E, Statistical, nonlinear, and soft matter physics.
[46] T. Henning,et al. Probing the evolution of molecular cloud structure: From quiescence to birth , 2009, 0911.5648.
[47] P. Hennebelle,et al. On the structure of the turbulent interstellar clouds . Influence of the equation of state on the dynamics of 3D compressible flows , 2009, 0911.0748.
[48] N. Peretto,et al. The initial conditions of star formation in the Ophiuchus main cloud: Kinematics of the protocluster condensations , , 2007, 0706.1535.
[49] E. Baron,et al. A 3D radiative transfer framework: IV. spherical & cylindrical coordinate systems , 2009, 0903.1949.
[50] M. Juvela,et al. The Power Spectrum of Supersonic Turbulence in Perseus , 2006, astro-ph/0611248.
[51] William H. Press,et al. Numerical recipes , 1990 .
[52] Coleman Krawczyk,et al. RE-EXAMINING LARSON'S SCALING RELATIONSHIPS IN GALACTIC MOLECULAR CLOUDS , 2008, 0809.1397.
[53] V. Ossenkopf,et al. Structure analysis of interstellar clouds - I. Improving the Delta-variance method , 2008, 0804.4649.
[54] J. Stone,et al. DISSIPATION AND HEATING IN SUPERSONIC HYDRODYNAMIC AND MHD TURBULENCE , 2008, 0809.4005.
[55] C. Brunt,et al. Turbulent Driving Scales in Molecular Clouds , 2009, 0910.0398.
[56] Enrico Camporeale,et al. Numerical modeling of space plasma flows , 2009 .
[57] A. Kravtsov. On the Origin of the Global Schmidt Law of Star Formation , 2003, astro-ph/0303240.
[58] Michael L. Norman,et al. The Formation of Self-Gravitating Cores in Turbulent Magnetized Clouds , 2003, astro-ph/0312622.
[59] Christopher F. McKee,et al. A General Theory of Turbulence-regulated Star Formation, from Spirals to Ultraluminous Infrared Galaxies , 2005, astro-ph/0505177.
[60] Two Regimes of Turbulent Fragmentation and the Stellar Initial Mass Function from Primordial to Present-Day Star Formation , 2007, astro-ph/0701795.
[61] A. Goodman,et al. Coherence in Dense Cores. II. The Transition to Coherence , 1998 .
[62] G. Kowal,et al. Density Fluctuations in MHD Turbulence: Spectra, Intermittency, and Topology , 2006, astro-ph/0608051.
[63] E. Feigelson,et al. A CHANDRA STUDY OF THE ROSETTE STAR-FORMING COMPLEX. II. CLUSTERS IN THE ROSETTE MOLECULAR CLOUD , 2009, 0903.5493.
[64] U. Texas,et al. Interstellar Turbulence II: Implications and Effects , 2004, astro-ph/0404452.
[65] A. Lazarian,et al. Statistics of Velocity from Spectral Data: Modified Velocity Centroids , 2003, astro-ph/0304007.
[66] James M. Stone,et al. Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models , 2000, astro-ph/0008454.
[67] C. Brunt,et al. Modification of Projected Velocity Power Spectra by Density Inhomogeneities in Compressible Supersonic Turbulence , 2003, astro-ph/0311461.
[68] P. Padoan,et al. The Stellar Initial Mass Function from Turbulent Fragmentation , 2000, astro-ph/0011465.
[69] James M. Stone,et al. Kinetic and Structural Evolution of Self-gravitating, Magnetized Clouds: 2.5-Dimensional Simulations of Decaying Turbulence , 1998, astro-ph/9810321.
[70] E. Ostriker,et al. Magnetically Aligned Velocity Anisotropy in the Taurus Molecular Cloud , 2008, 0802.2084.
[71] Embedding Lagrangian Sink Particles in Eulerian Grids , 2003, astro-ph/0312612.
[72] R. Klessen,et al. A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency: First Tests , 2003, astro-ph/0301546.
[73] Sebastian Kern,et al. Numerical simulations of compressively driven interstellar turbulence. I. Isothermal gas , 2008, 0809.1321.
[74] Mika Juvela,et al. The Super-Alfvénic Model of Molecular Clouds: Predictions for Zeeman Splitting Measurements , 2008, 0806.3854.
[75] Statistical Properties of Line Centroid Velocity Increments in the ρ Ophiuchi Cloud , 1998 .
[76] Structure Function Scaling in the Taurus and Perseus Molecular Cloud Complexes , 2002, astro-ph/0207568.
[77] DENSE CORES IN PERSEUS: THE INFLUENCE OF STELLAR CONTENT AND CLUSTER ENVIRONMENT , 2009, 0902.0536.
[78] The Energy Dissipation Rate of Supersonic, Magnetohydrodynamic Turbulence in Molecular Clouds , 1998, astro-ph/9809177.
[79] R. Klessen,et al. Quiescent and Coherent Cores from Gravoturbulent Fragmentation , 2003, astro-ph/0306055.
[80] P. Myers. Dense cores in dark clouds. III. Subsonic turbulence. , 1983 .
[81] V. Ossenkopf,et al. Structure analysis of interstellar clouds - II. Applying the Delta-variance method to interstellar turbulence , 2008, 0804.4877.
[82] Velocity field statistics in star-forming regions. I. Centroid velocity observations , 1998, astro-ph/9810427.
[83] D. Balsara,et al. The Distribution of Pressures in a Supernova-Driven Interstellar Medium , 2001, astro-ph/0106509.
[84] B. Elmegreen. Variations in Stellar Clustering with Environment: Dispersed Star Formation and the Origin of Faint Fuzzies , 2007, 0710.5788.
[85] F. Bensch,et al. Quantification of molecular cloud structure using the ∆ -variance , 2000 .
[86] Dynamic Cores in Hydrostatic Disguise , 2003, astro-ph/0304008.
[87] F. Bensch,et al. Quantification of molecular cloud structure using the Delta -variance , 2001 .
[88] P. Myers,et al. A survey for dense cores in dark clouds , 1989 .
[89] R. Klessen,et al. From the warm magnetized atomic medium to molecular clouds , 2008, 0805.1366.
[90] E. Pérez,et al. The Fractal Dimension of Projected Clouds , 2005, astro-ph/0501573.
[91] A. Vincent,et al. The spatial structure and statistical properties of homogeneous turbulence , 1991, Journal of Fluid Mechanics.
[92] Lawrence Livermore National Lab.,et al. Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars , 2008, 0806.1045.
[93] E. Vázquez-Semadeni. Hierarchical Structure in Nearly Pressureless Flows as a Consequence of Self-similar Statistics , 1994 .
[94] P. Woodward,et al. The Piecewise Parabolic Method (PPM) for Gas Dynamical Simulations , 1984 .
[95] Arrow,et al. The Physics of Fluids , 1958, Nature.
[96] H. Rix,et al. WHAT IS DRIVING THE H i VELOCITY DISPERSION? , 2009, 0903.0183.
[97] A. Tielens,et al. The neutral atomic phases of the interstellar medium , 1995 .
[98] E. Ostriker,et al. Theory of Star Formation , 2007, 0707.3514.
[99] Stanislav Boldyrev,et al. Scaling Relations of Supersonic Turbulence in Star-forming Molecular Clouds , 2001, astro-ph/0111345.
[100] Andreas Burkert,et al. Kinetic Energy Decay Rates of Supersonic and Super-Alfvénic Turbulence in Star-Forming Clouds , 1998 .
[101] C. McKee,et al. THE STAR FORMATION LAW IN ATOMIC AND MOLECULAR GAS , 2009, 0904.0009.
[102] V. Ossenkopf,et al. Turbulent velocity structure in molecular clouds , 2000, astro-ph/0012247.
[103] E. Baron,et al. A 3D radiative transfer framework: V. Homologous Flows , 2009, 0903.2486.
[104] R. Klessen,et al. Control of star formation by supersonic turbulence , 2000, astro-ph/0301093.
[105] B. Jones,et al. The universality of the stellar initial mass function , 1997 .
[106] R. Larson. Thermal physics, cloud geometry and the stellar initial mass function , 2005 .
[107] Daniel J. Price,et al. Algorithmic comparisons of decaying, isothermal, supersonic turbulence , 2008, 0810.4599.
[108] P. Padoan,et al. THE STAR FORMATION RATE OF SUPERSONIC MAGNETOHYDRODYNAMIC TURBULENCE , 2009, 0907.0248.
[109] B. Elmegreen. Star Formation from Galaxies to Globules , 2001, astro-ph/0207114.
[110] Porter,et al. Three-dimensional supersonic homogeneous turbulence: A numerical study. , 1992, Physical review letters.
[111] The Stellar Mass Spectrum from Non-Isothermal Gravoturbulent Fragmentation , 2004, astro-ph/0410371.
[112] B. Fryxell,et al. FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes , 2000 .
[113] Axel Brandenburg,et al. Inertial range scaling in numerical turbulence with hyperviscosity. , 2004, Physical review. E, Statistical, nonlinear, and soft matter physics.
[114] J. Francesco,et al. THE INITIAL CONDITIONS OF CLUSTERED STAR FORMATION. I. NH3 OBSERVATIONS OF DENSE CORES IN OPHIUCHUS , 2009, 0903.0690.
[115] J. Pety,et al. Statistical Properties of Line Centroid Velocities and Centroid Velocity Increments in Compressible Turbulence , 1996 .
[116] Hydrodynamical simulations of the decay of high-speed molecular turbulence – II. Divergence from isothermality , 2005, astro-ph/0504504.
[117] T. Henning,et al. Multiple low-turbulence starless cores associated with intermediate- to high-mass star formation , 2009, 0907.4565.
[118] P. Padoan,et al. Interstellar Turbulence: The Density PDFs of Supersonic Random Flows , 1999 .
[119] G. Kowal,et al. DENSITY STUDIES OF MHD INTERSTELLAR TURBULENCE: STATISTICAL MOMENTS, CORRELATIONS AND BISPECTRUM , 2008, 0811.0822.
[120] Interstellar cloud structure: the statistics of centroid velocities , 2006, astro-ph/0602265.
[121] Jongsoo Kim,et al. The Lifetimes and Evolution of Molecular Cloud Cores , 2005 .
[122] Turbulence in Molecular Clouds , 1995, astro-ph/9501032.
[123] Mordecai-Mark Mac Low,et al. The Formation of Stellar Clusters in Turbulent Molecular Clouds: Effects of the Equation of State , 2002, astro-ph/0210479.
[124] Volker Ossenkopf,et al. Statistics of velocity centroids: effects of density–velocity correlations and non‐Gaussianity , 2007 .
[125] Stephen B. Pope,et al. An examination of forcing in direct numerical simulations of turbulence , 1988 .
[126] M. Heyer,et al. Application of Principal Component Analysis to Large-Scale Spectral Line Imaging Studies of the Interstellar Medium , 1997 .
[127] Wolfram Schmidt,et al. THE FRACTAL DENSITY STRUCTURE IN SUPERSONIC ISOTHERMAL TURBULENCE: SOLENOIDAL VERSUS COMPRESSIVE ENERGY INJECTION , 2007, 0710.1359.
[128] C. Brunt,et al. The Universality of Turbulence in Galactic Molecular Clouds , 2004, astro-ph/0409420.
[129] M. Min,et al. Benchmark problems for continuum radiative transfer. High optical depths, anisotropic scattering, and polarisation , 2009, 0903.1231.
[130] K. Ferrière. The interstellar environment of our galaxy , 2001, astro-ph/0106359.
[131] J. Burgers. A mathematical model illustrating the theory of turbulence , 1948 .
[132] J. Scalo,et al. On the Probability Density Function of Galactic Gas. I. Numerical Simulations and the Significance of the Polytropic Index , 1997, astro-ph/9710075.
[133] James M. Stone,et al. Density Probability Distribution Functions in Supersonic Hydrodynamic and MHD Turbulence , 2008, 0806.1525.
[134] Gilles Chabrier,et al. Analytical Theory for the Initial Mass Function: CO Clumps and Prestellar Cores , 2008, 0805.0691.
[135] E. Falgarone,et al. A signature of the intermittency of interstellar turbulence - The wings of molecular line profiles , 1990 .
[136] I. Bonnell,et al. Fragmentation in Molecular Clouds and its connection to the IMF , 2009, 0903.3240.
[137] A. R. Rivolo,et al. Mass, luminosity, and line width relations of Galactic molecular clouds , 1987 .
[138] Paul R. Woodward,et al. A numerical study of supersonic turbulence , 1992 .
[139] R. Henriksen. On molecular cloud scaling laws and star formation , 1991 .
[140] Radiative transfer and starless cores , 2004, astro-ph/0407433.
[141] C. Brunt,et al. Intrinsic, Observed, and Retrieved Properties of Interstellar Turbulence , 2003 .
[142] Turbulent Gas Flows in the Rosette and G216-2.5 Molecular Clouds: Assessing Turbulent Fragmentation Descriptions of Star Formation , 2005, astro-ph/0511441.
[143] Mark S. Miesch,et al. Statistical Analysis of Turbulence in Molecular Clouds , 1994 .
[144] R. Larson. Turbulence and star formation in molecular clouds , 1980 .
[145] R. Klessen,et al. Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence , 2000, astro-ph/0009227.
[146] D. O. Astronomy,et al. Interstellar Turbulence I: Observations and Processes , 2004, astro-ph/0404451.
[147] Rainer Grauer,et al. Density-PDFs and Lagrangian statistics of highly compressible turbulence , 2008 .
[148] Jr. Fleck,et al. Scaling Relations for the Turbulent, Non--Self-gravitating, Neutral Component of the Interstellar Medium , 1996 .
[149] R. Klessen,et al. Is the scaling of supersonic turbulence universal? , 2008, Physical review letters.
[150] C. Brunt,et al. Interstellar Turbulence: I. Retrieval of Velocity Field Statistics , 2000, astro-ph/0011200.
[151] Ray Tracing for Complex Astrophysical High-opacity Structures , 2006, astro-ph/0603463.
[152] 2MASS wide field extinction maps. I. The Pipe nebula , 2006, astro-ph/0606670.
[153] On the structure of the turbulent interstellar atomic hydrogen. I- Physical characteristics Influence and nature of turbulence in a thermally bistable flow , 2006, astro-ph/0612778.
[154] October I. Physical Review Letters , 2022 .
[155] The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function , 2005, astro-ph/0509591.
[156] A. Goodman,et al. Coherent Dense Cores. I. NH3 Observations , 1998 .
[157] T. Naab,et al. DRIVING TURBULENCE AND TRIGGERING STAR FORMATION BY IONIZING RADIATION , 2009, 0901.2113.
[158] R. Klessen,et al. Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence , 1999, astro-ph/9911068.
[159] R. Klein,et al. Sub-Alfvénic Nonideal MHD Turbulence Simulations with Ambipolar Diffusion. I. Turbulence Statistics , 2008, 0805.0597.
[160] Kindler-Rohrborn,et al. In press , 1994, Molecular carcinogenesis.
[161] Numerical dissipation and the bottleneck effect in simulations of compressible isotropic turbulence , 2004, astro-ph/0407616.
[162] Ralf S. Klessen. One-Point Probability Distribution Functions of Supersonic Turbulent Flows in Self-gravitating Media , 2000 .
[163] On the structure of self-gravitating molecular clouds , 2001, astro-ph/0110453.
[164] Ralf Klessen,et al. (ACCEPTED FOR PUBLICATION IN APJ) Preprint typeset using L ATEX style emulateapj v. 04/03/99 THE FORMATION OF STELLAR CLUSTERS: MASS SPECTRA FROM TURBULENT MOLECULAR CLOUD , 2001 .