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– 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. 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Bec J, Gawedzki K, Horvai P. 2003. Supernova shock acceleration of cosmic rays in the Galaxy. ApJ. Cambridge: Cambridge Univ. Yanasak NE, Wiedenbeck ME, Mewaldt RA, Davis AJ, Cummings AC, George JS, Leske.
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