References from Interstellar Turbulence I: Observations and Processes
Authors: Bruce Elmegreen & John Scalo
Adler DS, Roberts WW Jr. 1992. Ambiguities in the identification of giant molecular cloud complexes from longitude-velocity diagrams. ApJ. 384:95-104
Andreopoulos Y, Agui JH, Briassulis G. 2000. Shock wave-turbulence interactions. Ann.Rev.Fluid Mech. 32:309-345
Anselmet F, Gagne Y, Jopfinger EJ, Antonia RA 1984. High order velocity structure functions in turbulent shear flows. J. Fluid Mech. 140:63-89
Arons J, Max CE. 1975. Hydromagnetic Waves in Molecular Clouds. ApJ. 196:L77-L81
Avila-Reese V, Vazquez-Semadeni E. 2001. Turbulent Dissipation in the Interstellar Medium: The Coexistence of Forced and Decaying Regimes and Implications for Galaxy Formation and Evolution. ApJ. 553:645-660
Ayyer A, Verma M. K. 2003. Energy transfer and locality in magnetohydrodynamic turbulence. ArXiv: nlin.CD/0308005
Baker PL. 1973. A Statistical Investigation of Neutral Hydrogen Line Profiles. A&A. 23:81-92
Balbus SA, Hawley JF. 1991. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution. ApJ . 376:214-222
Ballesteros-Paredes J. 2003. Turbulent Fragmentation and Star Formation Authors: Javier Ballesteros-Paredes. astroph/0311319
Ballesteros-Paredes J, Vazquez-Semadeni E, Scalo J. 1999. Clouds as Turbulent Density Fluctuations: Implications for Pressure Confinement and Spectral Line Data Interpretation. ApJ. 515:286-303
Ballesteros-Paredes J, Hartmann L, Vazquez-Semadeni E. 1999. Turbulent Flow-driven Molecular Cloud Formation: A Solution to the Post-T Tauri Problem? ApJ. 527:285-297
Ballesteros-Paredes J, Mac Low M-M. 2002. Physical versus Observational Properties of Clouds in Turbulent Molecular Cloud Models. ApJ. 570:734-748
Ballesteros-Paredes J, Vazquez-Semadeni E, Goodman, AA. 2002. Velocity Structure of the Interstellar Medium as Seen by the Spectral Correlation Function. ApJ. 571:334-355
Ballesteros-Paredes J, Klessen RS, Vazquez-Semadeni E. 2003. Dynamic Cores in Hydrostatic Disguise. ApJ. 592:188-202
Bally J, Langer WD, Stark AA, Wilson RW 1987. Filamentary structure in the Orion molecular cloud. ApJ. 312:L45-L49
Balsara D, Benjamin RA, Cox DP. 2001. The Evolution of Adiabatic Supernova Remnants in a Turbulent, Magnetized Medium. ApJ. 563:800-805
Balsara DS, Crutcher RM, Pouquet A. 2001. Turbulent Flows within Self-gravitating Magnetized Molecular Clouds. ApJ. 557:451-463
Balsara D, Ward-Thompson D, Crutcher RM. 2001. A turbulent MHD model for molecular clouds and a new method of accretion on to star-forming cores. MNRAS. 327:715-720
Bania TM, Lyon JG. 1980. OB stars and the structure of the interstellar medium - Cloud formation and effects of different equations of state. ApJ. 239:173-192
Barrat A, Trizac E. 2002. Molecular dynamics simulations of vibrated granular gases. Phys. Rev. E. 66:051303-1-051303-13
Basu S, Murali C. 2001. Constraints on Stirring and Dissipation of MHD Turbulence in Molecular Clouds. ApJ. 551:743-746
Bataille F, Zhou Y. 1999. Nature of the energy transfer process in compressible turbulence. Phys. Rev. E. 59:5417-5426
Bate MR, Burkert A. 1997. Resolution requirements for smoothed particle hydrodynamics calculations with self-gravity. MNRAS . 288:1060-1072
Bate MR, Bonnell IA, Bromm V. 2002. The formation of close binary systems by dynamical interactions and orbital decay. MNRAS. 336:705-713
Bate MR, Bonnell IA, Bromm V. 2003. The formation of a star cluster: predicting the properties of stars and brown dwarfs. MNRAS. 339:577-599
Bazell D, Desert FX. 1988. Fractal structure of interstellar cirrus. ApJ. 333:353-358
Beech M. 1987. Are LYNDS dark clouds fractals? Ap&SS. 133:193-195
Ben-Naim E, Krapivsky PL. 2002. Scaling, multiscaling, and nontrivial exponents in inelastic collision processes. Phys. Rev. E. 66:011309-1-011309-10
Bensch F, Stutzki J, Ossenkopf, V. 2001. Quantification of molecular cloud structure using the Delta -variance. A&A. 366:636-650
Beran MJ. 1968. Statistical continuum theories. New York: Interscience Publishers. 424 pp.
Berkhuijsen EM. 1999. Volume Filling Factors of ISM Phases and Turbulent Structure. In Plasma Turbulence and Energetic Particles in Astrophysics. ed. M Ostrowski, R Schlickeiser, pp. 61-65. Krakow: Obs. Astron. Uniw. Jagiellonski
Bertin G, Lodato G. 2001. Thermal stability of self-gravitating, optically thin accretion disks. A&A . 370:342-350
Bertoglio JP, Bataille F, Marion JD 2001. Two-point closures for weakly compressible turbulence. Phys. Fluids. 13:290-310
Bertoldi F, McKee CF. 1992. Pressure-confined clumps in magnetized molecular clouds. ApJ. 395:140-157
Bhattacharjee A, Ng CS. 2001. Random Scattering and Anisotropic Turbulence of Shear Alfven wave Packets. ApJ. 548:318-322
Biferale L. 2003. Shell models of energy cascade in turbulence. Ann. Rev. Fluid Mech. 35:441-468
Biferale L, Lanotte A, Toschi F. 2003. Effects of forcing in three dimensional turbulent flows. nlin.CD/0310022
Biskamp D 2003. Magnetohydrodynamic turbulence. Cambridge: Cambridge Univ. Press. 310 pp.
Biskamp D, Muller W-C. 1999. Decay Laws for Three-Dimensional Magnetohydrodynamic Turbulence. Phys.Rev.Lett. 83:2195-2198
Biskamp D, Muller W-C. 2000. Scaling properties of three-dimensional isotropic magnetohydrodynamic turbulence. Physics of Plasmas. 7:4889-4900
Biskamp D, Schwarz E. 2001. On two-dimensional magnetohydrodynamic turbulence. Phys. Plasmas 8:3282-3292
Black DC, Matthews MS. Eds. 1985 Protostars and Planets II. Tucson: Univ. Ariz. Press
Blondin JM, Marks BS. 1996. Evolution of cold shock-bounded slabs. NewA . 1:235-244
Bok BJ, Reilly EF. 1947. Small Dark Nebulae. ApJ. 105:255-257
Boldyrev, S. 2002. Kolmogorov-Burgers Model for Star-forming Turbulence. ApJ. 569:841-845
Boldyrev S. Nordlund A. Padoan P. 2002. Scaling Relations of Supersonic Turbulence in Star-forming Molecular Clouds ApJ. 573:678-684
Boldyrev S, Nordlund A, Padoan, P. 2002. Supersonic Turbulence and Structure of Interstellar Molecular Clouds. Phys. Rev. Lett. 89:031102-031102-4
Bonazzola S, Heyvaerts J, Falgarone E, Perault M, Puget JL. 1987. Jeans collapse in a turbulent medium. A&A. 172:293-298
Bonazzola S, Perault M, Puget JL, Heyvaerts J, Falgarone E, Panis, JF. 1992. Jeans collapse of turbulent gas clouds - Tentative theory. J. Fluid Mech. 245:1-28
Bonnell IA, Bate MR, Clarke CJ, Pringle JE. 1997. Accretion and the stellar mass spectrum in small clusters. MNRAS. 285:201-208
Bonnell IA, Bate MR, Vine SG. 2003. The hierarchical formation of a stellar cluster. MNRAS. 343:413-418
Bourke TL, Myers PC, Robinson G, Hyland AR. 2001. New OH Zeeman measurements of magnetic field strengths in molecular clouds. ApJ. 554:916-932
Bracco A, LaCasce J, Pasquero C, Provenzale A. 2000. The velocity distribution of barotropic turbulence. Phys. Fluids. 12:2478-2488
Brand J, Wouterloot JGA, Rudolph AL, deGeus EJ. 2001. Clumpy outer Galaxy molecular clouds and the steepening of the IMF. A&A. 377:644-671
Brandenburg A, Zweibel EG. 1994. The formation of sharp structures by ambipolar diffusion. ApJ. 427:L91-L94
Brandenberg A, Nordlund A, Stein RF, Torkelsson I. 1996. The Disk Accretion Rate for Dynamo-generated Turbulence. ApJ. 458:L45-L48
Brunt CM, Heyer MH. 2002. Interstellar Turbulence. II. Energy Spectra of Molecular Regions in the Outer Galaxy. ApJ. 566:289-301
Brunt CM, Heyer MH, Vazquez-Semadeni E, Pichardo B. 2003. Intrinsic, observed and retrieved properties of interstellar turbulence. ApJ. 595:824-841
Burkert A, Bodenheimer P. 2000. Turbulent molecular cloud cores: Rotational Properties. ApJ. 543:822-830
Burton WB. 1971. Galactic Structure Derived from Neutral Hydrogen Observations Using Kinematic Models Based on the Density-wave Theory. A&A. 10:76-96
Bunner AN, Coleman PL, Kraushaar WL, McCammon D. 1971. Low-Energy Diffuse X-Rays. ApJ. 167:L3-L8
Cambresy L. 1999. Mapping of the extinction in giant molecular clouds using optical star counts. A&A. 345:965-976
Caselli P. Walmsley CM, Zucconi A, Tafalla M, Dore L, Myers PC. 2002. Molecular Ions in L1544. I. Kinematics. ApJ. 565:331-343
Castaing B, Gagne Y, Hopfinger EJ 1990. Velocity probability density functions of high Reynolds number turbulence. Physica D. 46:177-200
Chabrier G. 2003. Galactic Stellar and Substellar Initial Mass Function. PASP. 115:763-795
Chandran BDG. 2003. A review of the theory of incompressible MHD turbulence In International Workshop on magnetic fields and star formation: theory versus observations. Dordrecht: Kluwer.
Chandrasekhar S, Munch G. 1952. The Theory of the Fluctuations in Brightness of the Milky way. V. ApJ. 115:103-123
Chappell D, Scalo J. 2001. Multifractal Scaling, Geometrical Diversity, and Hierarchical Structure in the Cool Interstellar Medium. ApJ. 551:712-729
Chavanis PH. 2002. Gravitational instability of finite isothermal spheres. A&A . 381:340-356
Chen H, Chen S, Kraichnan RH. 1989. Probability distribution of a statistically advected scalar field. Phys. Rev. Lett. 63:2657-2660
Chen H, Herring JR, Kerr RM, Kraichnan RH. 1989. Non-Gaussian statistics in isotropic turbulence. Phys. Fluids A. 1:1844-1854
Chen J-Y, Kollman W. 1994. In Turbulent Reacting Flows. ed. PA Libby, FA Williams. pp. 211-308. New York:Springer-Verlag. 474 pp.
Chen H, Kandasamy S, Orszag S, Shock R, Succi S, Yakhot V. 2003. Extended Boltzmann kinetic equation for turbulent flows. Science 301:633-636
Chen Q, Chen S, Eyink GL 2003. The joint cascade of energy and helicity in three-dimensional turbulence. Phys. Fluids. 15:361-374
Chen S, Doolen G, Herring JR, Kraichnan RH, Orszag SA, She ZS. 1993. Far dissipation range of turbulence. Phys. Rev. Lett. 70:3051-3054
Chen S, Kraichnan RH. 1997. Inhibition of turbulent cascade by sweep. J. Plasma Phys. 57:187-193
Chen S, Ecke RE, Eyink GL, Wang X, Xiao Z. 2003. Physical Mechanism of the Two-Dimensional Enstrophy Cascade. Phys. Rev. Letts. 91:214501-214501-4
Chew GF, Goldberger ML, Low FE. 1956. The Boltzmann equation and the one-fluid hydromagnetic equations in the absence of particle collisions. Proc. Roy. Soc. (London) A 236:112-118
Chiang W-H, Prendergast KH. 1985. Numerical study of a two-fluid hydrodynamic model of the interstellar medium and population I stars. ApJ. 297:507-530
Chiang W-H. Bregman JN. 1988. A model for the interaction between stars and gas in the interstellar medium. ApJ. 328:427-439
Cho J, Lazarian A, Vishniac ET. 2002a. Simulations of Magnetohydrodynamic Turbulence in a Strongly Magnetized Medium. ApJ. 564:291-301
Cho J, Lazarian A, Vishniac ET. 2002b. New Regime of Magnetohydrodynamic Turbulence: Cascade below the Viscous Cutoff. ApJ. 566:L49-L52
Cho J, Lazarian A. 2002a. Magnetohydrodynamic Turbulence as a Foreground for Cosmic Microwave Background Studies. ApJ. 575:L63-L66
Cho J, Lazarian A. 2002b. Compressible Sub-Alfvenic MHD Turbulence in Low-b Plasmas. Phys.Rev.Letts. 88:245001-245001-4
Cho J, Lazarian A. 2003c. Compressible Magnetohydrodynamic Turbulence: mode coupling, scaling relations, anisotropy, new regime and astrophysical implications. MNRAS. 345:325-339
Cho J, Lazarian A, Vishniac ET. 2003a. MHD turbulence: scaling laws and astrophysical implications. In Turbulence and magnetic fields in astrophysics. ed. T Passot, E Falgarone. Springer lecture notes in physics 614:56-100
Cho J, Lazarian A, Vishniac ET. 2003b. Ordinary and Viscosity-damped Magnetohydrodynamic Turbulence. ApJ. 595:812-823
Christensson M, Hindmarsh M, Brandenburg A. 2001. Inverse cascade in decaying three-dimensional magnetohydrodynamic turbulence. Phys Rev E. 64:056405-056405-6
Connaughton C, Nazarenko S, Newell AC. 2003. Dimensional analysis and weak turbulence. Physica D. 184:86-97
Court A. 1965. Undulence and turbulence. Quart. J. Roy. Meteor. Soc. 91:234-235
Clark BG. 1965. An Interferometer Investigation of the 21-centimeter Hydrogen-Line Absorption. ApJ. 142:1398-1422
Crovisier J, Dickey JM. 1983. The spatial power spectrum of galactic neutral hydrogen from observations of the 21-cm emission line. A&A. 122:282-296
Crutcher RM. 1999. Magnetic fields in molecular clouds: observations confront theory. ApJ. 520:706-713
Dame T, Elmegreen BG, Cohen R, Thaddeus P. 1986. The largest molecular cloud complexes in the first galactic quadrant. ApJ. 305:892-908
de Avillez MA. 2000. Disc-halo interaction - I. Three-dimensional evolution of the Galactic disc. MNRAS. 315:479-497
de Avillez MA, Berry DL. 2001. Three-dimensional evolution of worms and chimneys in the Galactic disc. MNRAS. 328:708-718
de Avillez MA, Breitschwerdt D. 2003a. High resolution simulations of the global and local ISM. In Star Formation through Time. ASP Conf. Series. ed. Perez, Gonzalez Delgado, Tenorio-Tagle (astro-ph/0303322)
de Avillez MA, Breitschwerdt D. 2003b. From Large to Small Scales: Global Models of the ISM. astro-ph/0310633
Delgado-Donate EJ, Clarke CJ, Bate MR. 2003. The dependence of the sub-stellar IMF on the initial conditions for star formation. MNRAS , in press (astro-ph/0310406)
Deiss BM, Just A, Kegel WH. 1990. Fluctuations of the interstellar medium induced by the stellar system: mechanical heating and dynamical friction. A&A. 240:123-136
Deshpande AA, Dwarakanath KS, Goss WM 2000. Power Spectrum of the Density of Cold Atomic Gas in the Galaxy toward Cassiopeia A and Cygnus. ApJ. 543:227-234
Dewan EM. 1985. On the nature of atmospheric waves and turbulence. Radio Sci. 20:1301-1307
Dickey JM. 1985. Small-scale structure and motions in the interstellar gas. In The Milky Way Galaxy. ed. H van Woerden, RJ Allen, WB Burton. pp. 311-317. Dordrecht: Reidel.
Dickey JM, Salpeter EE, Terzian, Y 1977, Temperature distribution of neutral hydrogen at high galactic latitudes. ApJ. 211:L77-L82
Dickey JM, Lockman FJ. 1990. H I in the Galaxy. ARAA. 28:215-261
Dickey JM, McClure-Griffiths NM, Stanimirovic S, Gaensler BM, Green AJ. 2001. Southern Galactic Plane Survey Measurements of the Spatial Power Spectrum of Interstellar H I in the Inner Galaxy. ApJ. 561:264-271
Dickman RL. 1985. Turbulence in molecular clouds. In Protostars and planets II. ed. DC Black, MS Matthews. pp. 150-174. Tucson:Univ. Ariz. Press
Dmitruk P, Gomez DO, Matthaeus WH. 2003. Energy spectrum of turbulent fluctuations in boundary driven reduced magnetohydrodynamics. astroph/0209111
Domaradzki JA, Rogallo RS. 1990. Local energy transfer and nonlocal interactions in homogeneous, isotropic turbulence. Phys. Fluids A. 2:413-426
Dopazo C. 1994. Recent developments in pdf methods. In Turbulent Reacting Flows, ed. PA Libby, FA Williams pp. 375-473. New York:Academic Press
Dopazo C, Valino L, Fueyo N. 1997. Statistical description of the turbulent mixing of scalar fields. Intern. J. Mod. Phys. B. 11:2975-3014
Dubinski J, Narayan R, Phillips TG. 1995. Turbulence in Molecular Clouds. ApJ. 448:226-231
Dubrulle B. 1994. Intermittency in fully developed turbulence: Log-Poisson statistics and generalized scale covariance. Phys.Rev.Letts. 73:959-962
Elmegreen BG. 1991. The Origin and Evolution of Giant Molecular Clouds. In The Physics of Star Formation and Early Stellar Evolution. Eds. CJ Lada, ND Kylafis. pp. 35-60
Elmegreen BG. 1993. Star Formation at Compressed Interfaces in Turbulent Self-gravitating Clouds. ApJ. 419:L29-L32
Elmegreen BG. 1999. Formation and Loss of Hierarchical Structure in Two-dimensional Magnetohydrodynamic Simulations of Wave-driven Turbulence in Interstellar Clouds. ApJ. 527:266-284
Elmegreen BG. 2000. Star Formation in a Crossing Time. ApJ. 530:277-281
Elmegreen BG, Elmegreen DM. 2001. Fractal Structure in Galactic Star Fields. AJ. 121:1507-1511
Elmegreen BG, Kim S, Staveley-Smith L. 2001. A Fractal Analysis of the H I Emission from the Large Magellanic Cloud. ApJ. 548:749-769
Elmegreen DM, Elmegreen BG, Eberwein KS. 2002. Dusty Acoustic Turbulence in the Nuclear Disks of Two LINER Galaxies NGC 4450 and NGC 4736. ApJ. 564:234-243
Elmegreen BG, Elmegreen DM, Leitner SN. 2003. A Turbulent Origin for Flocculent Spiral Structure in Galaxies. ApJ . 590:271-283
Esquivel A, Lazarian A, Pogosyan D, Cho J. 2003. Velocity statistics from spectral line data: effects of density-velocity correlations, magnetic field and shear. MNRAS. 342:325-336