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Table 2:

Derived parameters of the H I cores.
  $N_{\rm HI}$ s D $T_{\rm kin}$ $\langle n \rangle$ P $M_{H {\sc i}}$
  1018 cm-2 arcmin pc K ${\rm cm^{-3}}$ $K~{\rm cm^{-3}}$ $M_{\odot}$
Range 12-32 58-127 1.9-5.9 140-350 1.3-3.1 270-980 1-24
Median 16 78 2.6 240 2.3 560 4
Range 29-76 54-124 2-6 170-730 2.2-5.7 780-2440 7-32
Median 40 86 5 410 3.6 1500 16

Notes. The first two rows correspond to the cloud 116.2+23.6 observed with WSRT. The last two rows correspond to the cloud 115.0+23.9 observed with VLA. $N_{\rm HI}$ is the observed H I column density of the cores, s is the angular size, D is the spatial diameter. $T_{\rm kin}$ is the kinetic temperature. $\langle n \rangle$  is the volume H I density. P is the pressure of the H I gas. $M_{H {\sc i}}$ is the visible H I mass of the core.


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