Skip to main content
. Author manuscript; available in PMC: 2016 Feb 9.
Published in final edited form as: Astron Astrophys. 2015 Oct 1;582:L1. doi: 10.1051/0004-6361/201526255

Table 1.

Column densities and ratios.

Species Ng.s. (×l015) [cm−2] N Ratio
CH3OCH3 (DME) 600 ± 120a,b
CH3CH2OCH3 (tEME) ≤4.0 ± 0.8a DME/tEME ≥ 150
CH3CH2OCH2CH3 ≤1.0 ± 0.2a DME/Tt-DEE ≥ 600
(Tt-DEE) tEME/Tt-DEE ≥ 4
CH3OCHCH2 ≤0.5 ± 0.1a DME/cis-MVE ≥ 1200
(cis-MVE)†† tEME/cis-MVE ≥ 9
CH3OCOH (MF) 240 ± 50a,b,c
CH3CH2OCOH (EF) 2.0 ± 0.4a,d MF/EF ≃ 120
CH3OH (MetOH) 2700 ± 500b,e,f
CH3CH2OH (EtOH) 60 ± 10b,d,e MetOH/EtOH ≃ 45
Gt-CH3CH2CH2OH 1.0 ± 0.2e MetOH/PropOH ≃ 2700
(PropOH) EtOH/PropOH ≃ 60

Notes.

trans-trans diethyl ether.

††

cis methyl vinyl ether.

a

Position A; same physical parameters of the ALMA tEME model (see Sect. 3.1).

b

Three kinetic temperatures: 50 ± 10, 150 ± 30, and 250 ± 75 K.

c

b type lines fitted (a type lines are optically thick); another component has been included to properly fit the observed line profiles (vLSR = +9 km s−1, Δv = 4 km s−1, TK = 150 ± 30 K, Ng.s = (1.0 ± 0.2) × 1017cm−2).

d

trans+gauche.

e

Position B; assuming the same physical parameters of the ALMA Gt-n-propanol model (see Sect. 3.2).

f

12C/13C = 45 (Tercero et al. 2010).