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Table 8

Column density ratios and molecular abundances.

Molecule Orion-KL Sgr B2 G34.3+0.2 TMC-1
X R X R X R X R

CH2CHCN (2.0 ± 0.6) × 10-8 ... 6.2 × 10-8j ... 3.0 × 10-10n ... 1.0 × 10-9p ...
1.5 × 10-9a 6.0 × 10-8k
1.8 × 10-9b
CH3CN (1.0 ± 0.3) × 10-7d 0.20d 3.0 × 10-8k 0.40e ... ... 7.5 × 10-10p 1.3p
4.0 × 10-9a 0.39a 2.0k
7.8 × 10-9b 0.23b 3.4l
5.1 × 10-9c 1.7e 0.40m
0.18–1.8f 0.37o
0.48g
CH3CH2CN (1.8 ± 0.5) × 10-7h 0.11h 6.0 × 10-10k* 0.72e 1.0 × 10-8n 0.20n ... >2.00q
3.0 × 10-9a 0.50a 11l
9.8 × 10-9b 0.18b 0.67m
0.15e 1.7n
0.14f 0.40o
0.06g
HCCCN (7 ± 2) × 10-9i 2.9i 5.0 × 10-9k 0.13e ... ... 7.5 × 10-8p 0.01p
1.8 × 10-9a 0.86a 12k
1.6 × 10-9b 1.1b 61o
1.8 × 10-9c 2.11e
0.6-1.5f
0.16g
NH2CN (7 ± 2) × 10-11 286 9.0 × 10-11k* 1.4e ... ... ... ...
30e 14o

Notes. Abundances (X) and column density ratios between vinyl cyanide and some studied cyanides (R) in Orion-KL and other sources.

(†)

Values from this work.

(a)

Sutton et al. (1995), hot core, telescope beam ~13.7′′.

(b)

Blake et al. (1987), hot core, telescope beam ~30′′.

(c)

Persson et al. (2007), hot core, source size 10”.

(d)

Bell et al. (2014), hot core (different components between 5–10′′) + plateau (10′′).

(e)

Turner (1991).

(h)

Daly et al. (2013), hot core (4–10′′) and mix hot core-plateau (25′′).

(i)

Esplugues et al. (2013b) hot core (7–10′′) and plateau (20′′).

(k)

Nummelin et al. (2000) small source-size averaged.

(k*)

Nummelin et al. (2000) beam averaged.

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