1. Canup, R.M. and Ward, W.R. Formation of the Galilean Satellites: Conditions of Accretion, Astron. J., 2002, vol. 124, pp. 3404–3423.
2. Cassen, P. and Pettibone, D., Steady Accretion of a Rotating Fluid, Astrophys. J., 1976, vol. 208, pp. 500–511.
3. Dorofeeva, V.A. and Makalkin, A.B., Evolyutsiya rannei Solnechnoi sistemy. Kosmokhimicheskie i fizicheskie aspekty (Evolution of the Early Solar System. Cosmochemical and Physical Aspects), Moscow: URSS, 2004.
4. Herbert, F., Davis, D.R., and Weidenschilling, S.J., Formation and Evolution of a Circumterrestrial Disk: Constrains on the Origin of the Moon in Geocentric Orbit, Origin of the Moon, Hartmann, W.K., et al., Eds., Houston: LPI, 1986, pp. 701–730.
5. Makalkin, A.B., Dorofeeva, V.A., and Ruskol, E.L., Modeling the Protosatellite Circum-Jovian Accretion Disk: An Estimate of the Basic Parameters, Astron. Vestn., 1999, vol. 33, no. 6, pp. 518–526 [Sol. Syst. Res. (Engl. Transl.), vol. 33, no. 6, pp. 456–563].