– 1 – Interstellar Turbulence II: Implications and Effect Authors: John Scalo and Bruce Elmegreen REFERENCES Achterberg A. 1981. On the propagation of relativistic particles in a high beta plasma. A&A. 98:161-172 Achterberg A. 1990. Particle acceleration by an ensemble of shocks. A&A. 231:251-258 Achterberg A, Blandford RD, Reynolds SP, 1994. Evidence for enhanced MHD turbulence outside sharp-rimmed supernova remnants. A&A. 281:220-230 AguirreA,HernquistL,SchayeJ,WeinbergDH,KatzN,GardnerJ.2001.MetalEnrichment of the Intergalactic Medium at z=3 by Galactic Winds. ApJ. 560:599-605 ´ Andre MK, Oliveira CM, Howk JC, Ferlet R, D´esert J-M, H´ebrard G, Lacour S, des Etangs AL,Vidal-MadjarA,MoosHW.2003.OxygenGas-PhaseAbundanceRevisited.ApJ. 591:1000-1012 Andrievsky SM, Kovtyukh VV, Luck RE, L´epine JRD, Maciel WJ, Beletsky YuV. 2002. Using Cepheids to determine the galactic abundance gradient. III. First results for the outer disc. 2002. A&A. 392:491-499 Argast D, Samland M, Gerhard OE, Thielemann F-K. 2000. Metal-poor halo stars as tracers of ISM mixing processes during halo formation. A&A. 356:873-887 Armstrong JW, Rickett BJ, Spangler SR. 1995. Electron density power spectrum in the local interstellar medium. ApJ. 443:209-221 Aschenbach B, Leahy DA. 1999. ROSAT all-sky survey map of the Cygnus Loop: Overall structure and comparison with radio map. A&A. 341:602-609 Audouze J, Silk J. 1995. The First Generation of Stars: First Steps toward Chemical Evo- lution of Galaxies. ApJ. 451:L49-L52 Axford WI, Leer E, Skadron G. 1977. The acceleration of cosmic rays by shock waves. Proc. 15th Int. Cosmic-Ray Conf. Sofia: B’lgarska Akademiia na Naukite. 11:132-137 Baade W, Zwicky F. 1934. Cosmic Rays from Supernovae. Proc. Nat. Acad. Sci. 20:259-263 – 2 – Balkovsky E, Falkovich G, Fouxon A. 2001. Intermittent Distribution of Inertial Particles in Turbulent Flows. Phys. Rev. Lett.. 86:2790-2793 Balsara D, Benjamin RA, Cox DP. 2001. ApJ. The Evolution of Adiabatic Supernova Rem- nants in a Turbulent, Magnetized Medium. ApJ. 563:800-805 Bamba A, Yamazaki R, Ueno M, Koyama K. 2003. Small-Scale Structure of the SN 1006 Shock with Chandra Observations. ApJ. 589:827-837 Bateman NPT, Larson RB. 1993. The dispersal of iron through the interstellar medium. ApJ. 407:634-638 Begelman MC, Fabian AC. 1990. Turbulent mixing layers in the interstellar and intracluster medium. MNRAS. 244:26P-29P Bec J, Gawedzki K, Horvai P. 2003. Intermittent distribution of tracers advected by a com- pressible random flow. nlin.CD/0310015 Bell AR. 1978. The acceleration of cosmic rays in shock fronts. I. MNRAS. 182:147-156 Berezinskii VS, Bulanov SV, Ginzburg VL, Dogiel VA, Ptuskin VS 1990. Astrophysics of Cosmic Rays. Amsterdam:North Holland Bergin EA, Alves, J, Huard T, Lada CJ. 2002. N2H+ and C18O depletion in a cold dark cloud. ApJ. 570:L101-L104. BettensRPA,LeeH-H,HerbstE.1995.Theimportanceofclassesofneutral-neutralreactions in the production of complex interstellar molecules. ApJ. 443:664-674 Bhat NDR, Gupta Y,Rao AP. 1998. Pulsar Scintillation and the Local Bubble. ApJ. 500:262- 279 Bhat NDR, Gupta Y, Rao AP. 1999. Long-Term Scintillation Studies of Pulsars. II. Refrac- tive Effects and the Spectrum of Plasma Density Fluctuations. ApJ. 514:249-271 Bhat NDR, Rao AP, Gupta Y. 1999. Long-Term Scintillation Studies of Pulsars. I. Obser- vations and Basic Results. ApJS. 121:483-513 Bhat NDR, Gupta Y. 2002. Pulsar Scintillation in the Local Interstellar Medium: Loop I and Beyond. ApJ. 567:342-353 Bieber JW, Wanner W, Matthaeus WH. 1996. Dominant two-dimensional solar wind turbu- lence with implications for cosmic ray transport. J. Geophys. Res. 101:2511-2522 – 3 – BieberJW,MatthaeusWH.1997.PerpendicularDiffusionandDriftatIntermediateCosmic- Ray Energies. ApJ. 485:655-659 Black JH, van Dishoeck EF. 1991. Chemistry and Small-Scale Structure of Diffuse and Translucent Clouds. In Fragmentation of Molecular Clouds and Star Formation. ed. E Falgarone, F Boulanger, G. Duvert, pp. 139-150. Dordrecht: Kluwer. Blackman EG, Field GB. 2002. New Dynamical Mean-Field Dynamo Theory and Closure Approach. Phys. Rev. Lett. 89:265007-265007-4 Blackman EG, Field GB. 2003. A New Approach to Turbulent Transport of a Mean Scalar. Phys. Fluids. 15:L73-6 Blandford RD. Ostriker JP. 1980. Supernova shock acceleration of cosmic rays in the Galaxy. ApJ. 237:793-808 Blandford R, Narayan R. 1985. Low-frequency variability of pulsars. MNRAS. 213:591-611 Blandford R, Eichler D. 1987. Particle Acceleration at Astrophysical Shocks - a Theory of Cosmic-Ray Origin. Phys. Rep. 154:1-75 Boesgaard AM. 1989. Metallicity in galactic clusters from high signal-to-noise spectroscopy. ApJ. 336:798-807 Boffetta G, Celani A, Cristani A, Vulpiani A. 1999. Pair dispersion in synthetic fully devel- oped turbulence. Phys. Rev. E. 60:6734-6741 BoffettaG,SokolovIM.2002.AddtoarticlecollectionRelativeDispersioninFullyDeveloped Turbulence: The Richardson’s Law and Intermittency Corrections. Phys. Rev. Lett. 88:094501-094501-1 Boland W, deJong T. 1982. Carbon depletion in turbulent molecular cloud cores. ApJ. 261:110-114 Boldyrev S, Gwinn C. 2003. Scintillations and Lvy Flights through the Interstellar Medium. ApJ. 584:791-796 Bracco A, Chavanis PH, Provenzale A. 1999. Particle aggregation in a turbulent Keplerian flow. Phys. Fluids, 11:2280- Brandenburg A, Kapyla P, Mohammed A. 2003. Non-Fickian diffusion and tau- approximation from numerical turbulence. Phys. Fluids 16:1020-27 – 4 – Burke JR, Silk J. 1976. The dynamical interaction of a newly formed protostar with infalling matter - The origin of interstellar grains. ApJ. 210:341-364 Bykov AM, Toptygin IN. 1985. Shock Generation of Turbulence and Cosmic-Ray Diffusion in the Interstellar Medium. Sov.Ast.Lett. 11:75-78 Bykov AM, Toptygin IN. 1993. Kinetics of particles in strongly turbulent plasmas. Soviet Phys.Uspekhi. 36:1020-1052 Cameron AGW. 1973. Accumulation processes in the primitive solar nebula. Icarus. 18:407- 450 Caputo F, Marconi M, Musella I, Pont F. 2001. Pulsational constraints to the metallicity gradient in the Galactic disk. A&A. 263:413-422 Cartledge SIB, Meyer DM, Lauroesch JT. 2003. The Homogeneity of Interstellar Krypton in the Galactic Disk. ApJ. 597:408-413 CarraroG,Ng,YK,PortinariL.1998.OntheGalacticdiscage-metallicityrelation.MNRAS. 296:1045-1056 Casse F, Lemoine M, Pelletier G. 2002. Transport of cosmic rays in chaotic magnetic fields. Phys. Rev. D. 65:23002-23016 Cesarsky CJ. 1980. Cosmic ray confinement in the Galaxy. ARAA. 18:289-319 Chandran BDG. 2000a. Scattering of Energetic Particles by Anisotropic Magnetohydrody- namic Turbulence with a Goldreich-Sridhar Power Spectrum. Phy. Rev. Lett. 85:4656- 4659 Chandran BDG. 2000b. Confinement and Isotropization of Galactic Cosmic Rays by Molecular-Cloud Magnetic Mirrors When Turbulent Scattering Is Weak. ApJ. 529:513-535 Chandran BDG. 2001. The importance of anisotropic interstellar turbulence and molecular- cloudmagneticmirrorsforgalacticcosmic-raypropagation.Space Sci. Rev.99:271-280 Chandran BDG, Backer DC. 2002. Radio Wave Propagation through a Medium Containing Electron Density Fluctuations Described by an Anisotropic Goldreich-Sridhar Spec- trum. ApJ. 576:176-187 Chandran BDG, Maron JL. 2003a. Thermal conduction in galaxy-cluster plasmas and the divergence of neighboring magnetic field lines in strong magnetohydrodynamic tur- bulence. ApJ. 602:170-80 – 5 – Chandran BDG, Maron JL. 2003b. Acceleration of energetic particles by large-scale com- pressible magnetohydrodynamic turbulence. ApJ 603:23-7 Charnley SB. 1998. The chemical signature of magnetohydrodynamic waves in molecular clouds. MNRAS. 298:L25-L28 Charnley SB, Markwick AJ. 2003. Complex bifurcations in interstellar chemistry? A&A. 399. 583-587 Chen H, Chen S, Kraichnan RH. 1989. Probability distribution of a stochastically advected scalar field. Phys. Rev. Lett. 63:2657-2660 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 J, Bieber JW. 1993. Cosmic-ray anisotropies and gradients in three dimensions. ApJ. 405:375-389 Chen YQ, Nissen PE, Zhao G, Zhang HW, Benoni T. 2000. Chemical composition of 90 F and G disk dwarfs. A&AS, 141:491-506 Chiappini C, Matteucci F, Romano D. 2001. Abundance Gradients and the Formation of the Milky Way. ApJ. 554:1044-1058 Chuvilgin LG, Ptuskin VS. 1993. Anomalous diffusion of cosmic rays across the magnetic field. A&A. 279:278-297 Clegg AW, Fey AL, Lazio TJW. 1998. The Gaussian Plasma Lens in Astrophysics: Refrac- tion. ApJ. 496:253-266 Cordes, JM. 1986. Space velocities of radio pulsars from interstellar scintillations. ApJ. 311:183-196 Cordes JM, Weisberg JM, Boriakoff V. 1985. Small-scale electron density turbulence in the interstellar medium. ApJ. 288:221-247 Cordes JM, Wolszczan A. 1986. Multiple imaging of pulsars by refraction in the interstellar medium. ApJ. 307:L27-L31 Cordes JM, Pidwerbetsky A, Lovelace RVE. 1986. Refractive and diffractive scattering in the interstellar medium. ApJ. 310:737-767 – 6 – Cordes JM, Rickett BJ, Backer DC. eds., 1988, Radio Wave Scattering in the Interstellar Medium, American Institute of Physics Conference Report (New York: American Institute of Physics). Cordes JM, Rickett BJ. 1998. Diffractive Interstellar Scintillation Timescales and Velocities. ApJ. 507:846-860 Cunha K, Lambert DL. 1994. Chemical evolution of the Orion association. 2: The carbon, nitrogen,oxygen,silicon,andironabundancesofmain-sequenceBstars.ApJ.426:170- 191 Cutler DJ, Groom DE. 1991. Mayflower Mine 1500 GV detector - Cosmic-ray anisotropy and search for Cygnus X-3. ApJ. 376:322-334 de Avillez MA, Mac Low M-M. 2002. ApJ. Mixing Timescales in a Supernova-driven Inter- stellar Medium. 581:1047-1060 Decamp N, Le Bourlot J. 2002. Interstellar turbulent velocity fields: Scaling properties, synthesis and effects on chemistry. A&A. 389:1055-1067 DeharvengL,PenaM,CaplanJ,CosteroR.2000.OxygenandheliumabundancesinGalactic HII regions - II. Abundance gradients. MNRAS. 311:329-345 Desai KM, et al. 1992. A speckle hologram of the interstellar plasma. ApJ. 393:L75-L78 Desai KM, Fey AL. 2001. Anisotropic Interstellar Scattering toward the Cygnus Region. ApJS. 133:395-411 Dolginov AZ, Silant’ev NA. 1990. Diffusion and acceleration of charged particles in a com- pressible turbulent medium. A&A. 236:519-526 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 Doty SD, van Dishoeck EF, van der Tak FFS, Boonman AMS. 2002. Chemistry as a probe of the structures and evolution of massive star-forming regions. A&A. 389. 446-463 Draine BT. 1985. Grain evolution in dark clouds. In Protostars and Planets II. ed. D. Black, M. Mathews. pp. 621-640. Tucson: Univ. Ariz. Press – 7 – Draine BT, Katz N. 1986. Magnetohydrodynamic shocks in diffuse clouds. II. Production of CH+, OH, CH, and other species. ApJ. 310:392-407 Dr¨oge, W. 1994. Transport of solar energetic particles. ApJS. 90:567-576 Drury LO’C, Ellison DE, Aharonian FA, Berezhko E, Bykov A, Decourchelle A, Diehl R, Meynet G, Parizot E, Raymond J, Reynolds S, Spangler S. 2001. Test of galactic cosmic-ray source models - Working Group Report. Space Sci. Rev. 99:329-352 Duffy P, Kirk JG, Gallant YA, Dendy RO. 1995. Anomalous transport and particle acceler- ation at shocks. A&A. 302:L21-L24 Edmunds MG. 1975. Is the galactic disk well mixed. Ap&SS. 32:483-491 Edvardsson B, Andersen J, Gustafsson B, Lambert DL, Nissen PE, Tomkin J. 1993. The Chemical Evolution of the Galactic Disk - Part One - Analysis and Results. A&A. 275:101-152 Elitzur M, Watson WD. 1980. Interstellar shocks and molecular CH/+/ in diffuse clouds. ApJ. 236:172-181 Elliot FW, Majda AJ. 1996. Pair dispersion over an inertial range spanning many decades. Phys. Fluids. 8:1052-1060 Ellison DC, Baring MG, Jones FC. 1995. Acceleration Rates and Injection Efficiencies in Oblique Shocks. ApJ. 453:873-882 ElmegreenBG.1998.Small-ScaleMixingoftheElements.InAbundanceProfiles: Diagnostic Tools for Galaxy History, ASP Conf. Ser. Vol. 147. ed. D Friedli, MG Edmunds, C Robert, L Drissen. pp. 278-286. Engelmann JJ, Ferrando P, Soutoul A, Goret P, Juliusson E. 1990. Charge composition and energy spectra of cosmic-ray nuclei for elements from Be to NI - Results from HEAO-3-C2. A&A. 233:96-111 Erlykin AD, Lagutin AA, Wolfendale AW. 2003. Properties of the interstellar medium and the propagation of cosmic rays in the Galaxy. Astrophys. Particles, 19:351-362 Falgarone E, Puget J-L. 1995. Intermittency of turbulence in interstellar clouds: implications forthegastemperatureanddecouplingofheavyparticlesfromthegasmotions.A&A. 293:840-852 – 8 – Falgarone E, Pineau des Forets G, Roueff E. 1995. Chemical signatures of the intermittency of turbulence in low density interstellar clouds. A&A. 300:870-880 Falkovich G, Gawedzki K, Vergassola M. 2001. Particles and fields in fluid turbulence. Rev. Mod. Phys. 73:913-976 Fedorov YuI, Kats MF, Kichatinov LL, Stehlik M. 1992. Cosmic-ray kinetics in a random anisotropic reflective non-invariant magnetic field. A&A. 260:499-509 Felice GM, Kulsrud RM, 2001. Cosmic-Ray Pitch-Angle Scattering through 90◦. ApJ. 553:198-210 Feltzing S, Gonzalez G. 2001. The nature of super-metal-rich stars. Detailed abundance analysis of 8 super-metal-rich star candidates. A&A. 367:253-265 Fermi E. 1949. On the Origin of the Cosmic Radiation. Phys. Rev. 75:1169-1174 Fermi E. 1954. Galactic Magnetic Fields and the Origin of Cosmic Radiation. ApJ. 119:1-6 Ferrara A, Pettini M, Shchekinov Y. 2000. Mixing metals in the early Universe. MNRAS. 319:539-548 Ferrari A, Masani A. 1985. Interstellar and intracluster tunnels - Acceleration of cosmic rays above 1015 eV. A&A. 152:205-212 Fessler, JR, Kulick JD, Eaton JK 1994. Preferential concentration of heavy particles in a turbulent channel flow. —it Phys.Fluids 6:3742-3749 Fiedler, et al. 1987. Daily observations of compact extragalactic radio sources at 2695 and 8085 MHz, 1979-1985. ApJS. 65:319-384 Fiedler R, Dennison B, Johnston KJ, Waltman EB, Simon RS. 1994. A summary of extreme scattering events and a descriptive model. ApJ. 430:581-594 Fields BD, Turan JW, Cowan JJ. 2002. A Simple Model for r-Process Scatter and Halo Evolution. ApJ. 575:845-854 Fisk LA. 1976. Solar modulation of galactic cosmic rays. IV - Latitude-dependent modula- tion. JGR. 81:4633-4650 Flower DR, Pineau des Forets G. 1998. C-type shocks in the interstellar medium: profiles of CH+ and CH absorption lines. MNRAS. 297:1182-1188 Foote EA, Kulsrud RM. 1979. Hydromagnetic waves in high Beta plasmas. ApJ. 233:302-316 – 9 – FosalbaP,LazarianA,PrunetS,TauberJA.2002.StatisticalPropertiesofGalacticStarlight Polarization. ApJ. 564:762-772 Friel ED, Boesgaard AM. 1992. Chemical composition of open clusters. III - Iron and carbon in F dwarfs in Coma, Praesepe, and M67. ApJ. 387:170-180 Frail DA, Diamond PJ, Cordes JM, van Langevelde HJ. 1994. Anisotropic scattering of OH/IR stars toward the Galactic center. ApJ. 427:L43-L46 Frisch U. 1995. Turbulence. Cambridge: Cambridge Univ. Press. pp. 296 Fung JCH, Vassilicos JC. 1998. Two-particle dispersion in turbulent-like flows. Phys. Rev. E. 57:1677-1690 Garnett DR, Kobulnicky HA. 2000. Distance Dependence in the Solar Neighborhood Age- Metallicity Relation. ApJ. 532:1192-1196 Gerola H, Glassgold AE. 1978. Molecular evolution of contracting clouds - Basic methods and initial results. ApJS. 37:1-25 Getmantsev GG. 1963. On the Isotropy of Primary Cosmic Rays. Sov. Astron. 6:477-479 Giacalone J, Jokipii JR. 1999. The Transport of Cosmic Rays across a Turbulent Magnetic Field. ApJ. 520:204-214 Ginzburg V, Syrovatskii SI. 1964. The Origin of Cosmic Rays, trans. HSH Massey, D ter Haar. New York: MacMillan Goldstein ML, Roberts DA, Matthaeus WH. 1995. Magnetohydrodynamic Turbulence In The Solar Wind. ARAA. 33:283-326 Gredel R. 1997. Interstellar CH+ in southern OB associations. A&A. 320:929-944 GredelR.1999.InterstellarC absorptionlinestowardsCH+formingregions.A&A.351:657- 2 668 Gredel R, Pineau des Forˆets G, Federman SR. 2002. Interstellar CN toward CH+-forming regions. A&A. 389:993-1014 Gupta Y. 1995. On the Correlation between Proper Motion Velocities and Scintillation Ve- locities of Radio Pulsars. ApJ. 451:717-723 Gupta Y, Bhat NDR, Rao AP. 1999. Multiple Imaging of PSR B1133+16 by the Interstellar Medium. ApJ. 520:173-181 – 10 – Hasselmann K, Wibberenz G. 1968. Scattering of Charged Particles by Random Electromag- netic Fields. Zs. f. Geophys. 34:353-388 Hall DE, Sturrock PA. 1967. Diffusion, scattering and acceleration of particles by stochastic electromagnetic fields. Phys. Fluids. 10:2620-2628 Hall AN. 1980. On the origin of long time-scale pulsar scintillations - I. cosmic ray streaming or the mirror instability? MNRAS. 190:353-369 Harrison PA, Lyne AG. 1993. Pulsar Velocities and the Scaleheight of Scattering in the Galaxy. MNRAS. 265:778-780 Heiles C. 1996. A Comprehensive View of the Galactic Magnetic Field, Especially near the Sun. In ASP Conf. Ser. 97, Polarimetry of the Interstellar Medium. ed. WG Roberge, DCB Whittet. pp.457-474. San Francisco:ASP Henry RRC, Worthey G. 1999. The Distribution of Heavy Elements in Spiral and Elliptical Galaxies. PASP. 111:919-945 Herbst E. 1999. Chemical Processes in Interstellar Space. In Millimeter Wave Astronomy: Molecular Physics. in Space. ed. WF Wall, A Carramin˜ana, L Carrasco. pp. 341-354. Dordrecht: Kluwer. Herr S, Wang L-P, Collins LR. 1996. EDQNM model of a passive scalar with a uniform mean gradient. Phys. Fluids. 8:1588-1608 Hewish A. 1980. Frequency-time structure of pulsar scintillation. MNRAS. 192:799-804 Hewish A. 1992. Pulsar scintillation as a physical tool. Philos. Trans. R. Soc. London. A341:167-176 Higdon JC, Lingenfelter RE. 2003. The Myriad-Source Model of Cosmic Rays. I. Steady State Age and Path Length Distributions. ApJ. 582:330-341 Hill AS, Stinebring DR, Barnor HA, Berwick DE, Webber AB. 2003. Pulsar scintillation arcs. I. frequency dependence. ApJ., 599:457-64 Holman GD, Ionson JA, Scott JS. 1979. Particle streaming - Is the Alfv´en velocity the ultimate speed limit. ApJ. 228:576-581 Hollenbach DJ, McKee C. 1979. Molecule formation and infrared emission in fast interstellar shocks. I. Physical processes. ApJS. 41:555-592
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