Arquivo do trabalho - IAG - USP

REFERÊNCIASSimon, R. 1965, AnAp, 28, 625Spaans, M. & Silk, J., 2000, ApJ, 538, 115Spitzer, L., Jr. 1968, Nebulae and Interstellar Matter, 1Stahter, S. W. 1983, ApJ, 268, 155Steffen W., López J. A., 2004, ApJ, 612, 319Stone, J. M., Gardner, T. A., Teuben, P., Hawley, J. F. & Simon, J. B., 2008, ApJ, 178,137Stone, J. M., & Zweibel, E. G. 2010, ApJ, 724, 131Strittmatter, P. A. 1966, MNRAS, 132, 359Sweet, P. A. 1958, Electromagn. Phenom. Cosm. Phys., 6, 123Tassis, K., & Mouschovias, T. C. 2005, ApJ, 618, 769Tenorio-Tagle G., Rozyczka M., 1986, å, 155, 120Toro, Eleuterio F.,Riemannsolversandnumerical methodsforfluiddynamics. Apracticalintroduction. Second edition. Springer-Verlag, Berlin, 1999. 624 pp.Umebayashi, T. & Nakano, T. 1980, PASJ, 32, 405Uzdensky, D. A., & Kulsrud, R. M. 2000, Phys. of Plasmas, 7, 4018Vazquez-Semadeni, E., Ostriker, E. C., Passot, T., Gammie, C. F., & Stone, J. M. 2000,Protostars and Planets IV, 3Vázquez-Semadeni, E., Kim, J., & Ballesteros-Paredes, J. 2005, ApJ, 630, L49Vázquez-Semadeni, E. 2010, Astronomical Society of the Pacific Conference Series, 438,83Vishniac, E. T., & Lazarian, A. 1999, ApJ, 511, 193156