Skip to main content
. 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 2. Observed line parameters of HCCCCNC in TMC-1.

J u vobsa
(MHz)
TA* b
(mK)
Δvc(kms–1) TA*dv d
(mK kms–1)
12 33628.151±0.010 3.6±0.5 0.71±0.12 2.68±0.3
13 36430.429±0.010 3.8±0.5 0.66±0.09 2.68±0.3
14 39232.730±0.010 3.1±0.6 0.85±0.12 2.76±0.3
15 42035.040±0.010 3.7±1.0 0.47±0.14 2.08±0.4
16 44837.295±0.010 4.9±1.2 0.42±0.19 2.24±0.5

Notes.

(a)

Observed frequencies for a vLSR of 5.83 km s–1. The J= 17-16 line has not been detected within a 3σ level of 5.7 mK.

(b)

Antenna temperature in mK.

(c)

Linewidth at half intensity derived by fitting a Gaussian line profile to the observed transitions (in kms–1).

(d)

Integrated line intensity in mK kms–1.