1. Ferriere, K.M.: The interstellar environment of our galaxy. Rev. Mod. Phys. 73, 1031–1066 (2001)
2. Vázquez—Semandeni, E., Ostriker, E.C., Passot, T., Gammie, C.F., Stone, J.M.: Compressible MHD turbulence: implications for molecular cloud and star formation. In: Mannings, V. et al. (eds.), Protostars and Planets IV, University of Arizona, Tucson, pp. 3–28 (2000)
3. Beuther, H., Ragan, S.E., Johnston, K., Henning, T., Hacar, A., Kainulainen, J.T.: Filament fragmentation in high-mass star formation. A&A 584(A67), 1–12 (2015)
4. Truelove, J.K., Klein, R.I., McKee, C.F., Holliman, J.H., Howell, L.H., Greenough, J.A., Woods, D.T.: Self-gravitational hydrodynamics with 3-D adaptive mesh refinement: methodology and applications to molecular cloud collapse and fragmentation. ApJ 495, 821 (1998)
5. Bate, M.R., Bonnell, I.A., Price, N.M.: Modeling accretion in protobinary systems, monthly notices of the royal astronomical society. MNRAS 277(2), 362–376 (1995)