Physical parameters from ammonia for the cores.
|(K)||( × 1014 cm-2)||(pc)||(M⊙)||(M⊙)|
Derived from interferometric observations of: millimetre continuum (C1, C1-a, C1-b and C2, Paper II), N2D+ (N and S, Paper I), and ammonia (A1, A2 and C3 this work);
from the 225 GHz continuum integrated emission (Paper II), assuming that Trot equals the dust temperature and a gas-to-dust ratio of 100;
from the 284 GHz continuum integrated emission (Paper II), assuming that Trot equals the dust temperature and a gas-to-dust ratio of 100;
from the 284 GHz continuum integrated emission, assuming a hot core temperature of 200 K (Paper II) and a gas-to-dust ratio of 100;
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