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. Author manuscript; available in PMC: 2020 Nov 24.
Published in final edited form as: Astron Astrophys. 2020 Oct 7;642:L8. doi: 10.1051/0004-6361/202039274

Table 1. Column densities and abundance ratios for the isomers of HC3N and HC5N towards TMC-1 and IRC+10216.

Molecule TMC-1 IRC+10216
N(HC3N) (2.3±0.2)×1014 (4.5±0.2)×1014
N(HCCNC) (3.0±0.3)×1012 (1.1±0.1)×1012
N(HNCCC) (5.2±0.3)×1011 (3.4±0.2)×1011
N(HC5N) (1.8±0.2)×1014 (4.2±0.4)×1014 b
N(HC4NC) (3.0±0.7)×1011 ≤2.1×1011
N(HNC5) ≤1.5×1011 ≤1.1×1011
N(HC7N) (6.4±0.2)×1013 (1.9±0.2)×1014 c
N(HC6NC) ≤9.0×1010 ≤2.0×1011
N(HC3N)/N(HCCNC) 77.0±8.0 392±22
N(HC3N)/N(HNCCC) 442.0±70.0 1305±45
N(HCCNC)/N(HNCCC) 5.8±1.0 4.0±0.9
N(HC5N)/N(HC4NC) 600±70.0 ≥2000
N(HC5N)/N(HNC5) ≥1200 ≥3800
N(HC4NC)/N(HNC5) ≥2 ≥1.9
N(HC7N)/N(HC6NC) ≥710.0 ≥950
N(HC3N)/N(HC5N) 1.3±0.2 1.1±0.2
N(HC5N)/N(HC7N) 2.8±0.3 2.2±0.5

Notes.

(a)

All column densities are given in units of cm–2.

(b)

For IRC+10216, we adopted the value derived by Pardo et al. (2020), which corresponds to the gas component with T rot=10.1 K. A second component, with similar column density, was found for high-J levels with a T rot=24.5 K.

(c)

For IRC+10216, we adopted the value derived by Pardo etal. (2020), which corresponds to the gas component with T rot=16.8 K. A second component, with a column density 2.5 lower, was found for high-J levels with a T rot=31.6 K.