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Table 4

The three input parameters, the resulting velocity dispersion σv, derived from the modeled collapse spectra, and the expected total velocity dispersion, following the found relation with m.

Fig. 29 m p area σv σcrit,nt
M pc−1 km s−1 km s−1
a 100 1.5 All 1.03 0.46
b 500 1.5 All 2.29 1.04
c 1000 1.5 All 3.23 1.47
d 500 2.0 All 2.65 1.04
e 500 3.0 All 3.24 1.04
f 500 1.5 Middle 2.86 -
g 500 1.5 Edge 0.62 -

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