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

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Table C.1

MADCUBAIJ best fits of the COMs detected in the GBT spectra.

	EG	ET	MF


log N_b (cm^-2)	15.1	15.5	16.1
log N_s (cm^-2)	17.9	17.7	18.1
T_ex (K)^a	147^b/142^b	89/76	147/142
v_LSR (km s^-1)	97.0	99.0	97.5
Δv (km s^-1)	5.5	5.4	5.3

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

^(b)

Since the energy range covered by the transitions is very narrow, we have fixed the temperature to the values obtained for MF.

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