Abstract
This article describes some of the techniques used to include various micro-processes in numerical gas-dynamic simulations. These techniques are then used in simulations of photo-evaporating clumps, H2 level populations and time dependent shocks/jets.
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Bertoldi, F. and McKee, C.F.: 1990, ApJ 354, 529.
Biro, S., Raga, A.C. and Cantó, J.: 1979, MNRAS 275, 557.
Davis, C.J., Eislöffel, J. and Smith, M.D.: 1996, ApJ 463, 236.
Eislöffel, J., Smith, M.D. and Davis, C.J.: 2000, A&A 359, 1147.
Falle, S.A.E.G.: 2002, ApJ 577, L123.
Hartigan, P., Curiel, S. and Raymond, J.C.: 1989, ApJL 347, L31.
Hartquist, T.W. and Dyson, J.E.: 1987, MNRAS 228, 957.
Hollenbach, D. and McKee, C.F.: 1979, ApJS 41, 555.
Mellema, G., Raga, A.C., Canto, J., Lundqvist, P., Balick, B., Steffen, W. and Noriega-Crespo, A.: 1998, A&A 331, 335.
Reipurth, B., Yu, K.C., Rodríguez, L.F., Heathcote, S. and Bally, J.: 1999, A&A 352, L83.
Smith, M.D. and Brand, P.W.: 1990, MNRAS 245, 108.
Toro, E.N.: 1978m Riemann Solvers and Numerical Methods for Fluid Dynamics, Springer-Verlag.
van Zadelhoff, G.J., Dullemond, C.P., Yates, J., van der Tak, F., Doty, S., Ossenkopf, V. Hogerheijde, M., Wiesemeyer, H., Juvela, M. and Schöier, F.: 2002, A&A, submitted.
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Lim, A. Gas-Dynamical Models of Star-forming Regions. Astrophysics and Space Science 285, 745–759 (2003). https://doi.org/10.1023/A:1026177714099
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DOI: https://doi.org/10.1023/A:1026177714099