. . . . . "5"^^ . "4" . "Palou\u0161, Jan" . . "RIV/67985815:_____/11:00371959!RIV12-AV0-67985815" . . "[7F5A0A304C6D]" . "The fragmentation of expanding shells - III. Oligarchic accretion and the mass spectrum of fragments"@en . "3"^^ . . "Smith, R. J." . "We use smoothed particle hydrodynamics (SPH) simulations to investigate the gravitational fragmentation of expanding shells through the linear and non-linear regimes. The results are analysed using spherical-harmonic decomposition to capture the initiation of structure during the linear regime, the potential-based method of Smith et al. to follow the development of clumps in the mildly non-linear regime and sink particles to capture the properties of the final bound objects during the highly non-linear regime. In the early, mildly non-linear phase of fragmentation, we find that the clump mass function still agrees quite well with the mass function predicted by the analytic model." . "GB - Spojen\u00E9 kr\u00E1lovstv\u00ED Velk\u00E9 Brit\u00E1nie a Severn\u00EDho Irska" . "P(LC06014), Z(AV0Z10030501)" . . "11"^^ . "200304" . . "Dale, James E." . . "stars formation; ISM bubbles; H II regions"@en . . . "Monthly Notices of the Royal Astronomical Society" . . . "Dale, James E." . "RIV/67985815:_____/11:00371959" . "10.1111/j.1365-2966.2010.17844.x" . "411" . "The fragmentation of expanding shells - III. Oligarchic accretion and the mass spectrum of fragments"@en . "000287859200010" . "0035-8711" . "We use smoothed particle hydrodynamics (SPH) simulations to investigate the gravitational fragmentation of expanding shells through the linear and non-linear regimes. The results are analysed using spherical-harmonic decomposition to capture the initiation of structure during the linear regime, the potential-based method of Smith et al. to follow the development of clumps in the mildly non-linear regime and sink particles to capture the properties of the final bound objects during the highly non-linear regime. In the early, mildly non-linear phase of fragmentation, we find that the clump mass function still agrees quite well with the mass function predicted by the analytic model."@en . "W\u00FCnsch, Richard" . . "The fragmentation of expanding shells - III. Oligarchic accretion and the mass spectrum of fragments" . "The fragmentation of expanding shells - III. Oligarchic accretion and the mass spectrum of fragments" . . "Whitworth, A." . . .