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Bouy, Herve (2004): Fundamental Properties of very low mass star and brown dwarf binaries. Dissertation, LMU München: Fakultät für Physik

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Figure

Table 1.The lithium test
Figure 3 Star formation numerical simulations of Bate et al. (2003). This simulation followed
Figure 4 Left image:Right images:University); NASA)gas away from the outside layers of the proplyds
Figure 5 Snapshots of the numerical simulations of Mayer et al. (2002) showing a 200 000 parti-cles disk of material around a young star
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