Formation of ethylene glycol and other complex organic molecules in star-forming regions

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Table C.2

MADCUBAIJ best fits of the SMA compact spectra towards the peak of the continuum for the different molecules.

	EG	ET	GA	MF	DME


log N_b (cm^-2)	16.3	17.2	16.0	17.5	17.7
log N_s (cm^-2)	17.7	17.7	17.4	17.9	18.7
T_ex (K)^a	88/75	187/184	165^a	240/243	113/105
v_LSR (km s^-1)	97.2	97.0	97.0	97.0	97.2
Δv (km s^-1)	5.2	5.9	6.0	6.4	7.6

Notes. The parameters of this table have been used to produce the synthetic spectra of Fig. 2.

^(a)

The first temperature corresponds to the beam-average value, while the second is the source-average value obtained assuming the source diameter given in Table 5.

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