Figure 17
Distribution of the specific angular momenta, j, for protostars. (a)–(d) Show JK04’s model M6k2 with different star formation efficiencies: (a) 15, (b) 30, (c) 45 and (d) 60 per cent. (e) Binaries among nearby G stars of Duquennoy & Mayor (1991). (f) Binaries in Taurus (Simon 1992). (g) and (h) Show the distributions from paper for the clfind and gaussclumps designations, respectively, decomposed according to the designations of HFR07.

Distribution of the specific angular momenta, j, for protostars. (a)–(d) Show JK04’s model M6k2 with different star formation efficiencies: (a) 15, (b) 30, (c) 45 and (d) 60 per cent. (e) Binaries among nearby G stars of Duquennoy & Mayor (1991). (f) Binaries in Taurus (Simon 1992). (g) and (h) Show the distributions from paper for the clfind and gaussclumps designations, respectively, decomposed according to the designations of HFR07.

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