## Appendix A: computing the fractal dimensionBy fractal dimension we mean more accurately the correlation fractal dimension. We will use the notation , defined as follows: if we consider a fractal set of points of equal weight located at , the fractal dimension of the ensemble obeys the relation: The brackets stand for an ensemble average. In computational applications and in physical systems, the limit is not reached. However the relation should hold at scales where the boundary effects created by the finite size of the system are negligible. In practice, for a non-fractal ensemble of points,
usually depends on
According to the definition, the computation of the fractal
dimension is based on the following method.
is the mean mass in a sphere of
radius ## Appendix B: clump mass spectrumAlthough the results are not very conclusive, we give the mass distribution of the clumps in the 3-D simple freefall, to allow comparison with observational data and other numerical simulations. Plotting against , the slope infered from observation data is -0.5. Thus the clump mass spectrum behaves as a power law: . To produce the mass spectrum, the first step is to define individual clumps. We have used an algorithm very similar to the one proposed by Williams et al. (1994). We compute the density field from an interpolation of the distribution of the particles with a cloud-in-cell scheme. It should be mentione d that this procedure tends to produce an artificially high number of very small clumps associated to isolated particles or pair of particules which should not be considered as clumps at all. On Fig. B.1 the clump mass spectrum is given at different times of the evolution and for the two types of initial conditions (). Quasi-periodic boundary conditions are used. As time increases, as we can see, the clump mass spectrum slope decreases to reach for and for . At later times, the power law is broken by the final dissipative collapse. According to this diagnosis, the case is closer to the observed values. However, once again, this simulation provides only a transient state which is unlikely to be a good model of a GMC.
© European Southern Observatory (ESO) 2000 Online publication: August 23, 2000 |