Skip to main content
. Author manuscript; available in PMC: 2021 Apr 6.
Published in final edited form as: Astron Astrophys. 2021 Feb 5;646:L7. doi: 10.1051/0004-6361/202040076

Table 1. Observed line parameters for CH3CO+ in TMC-1.

Ju K vobsa
(MHz)
Δvocb
(kHz)
TAc
(mK)
Δvd
(kms−1)
TAdve
(mK km s−1)
2 0 36537.765 -3.5 39.O±O.6 0.63±0.01 26.1±0.6
2 1 36537.014 -0.6 11.8±O.6 0.60±0.03 7.5±0.6
4 0 73074.769 2.7 71.0±3.5 0.47±0.03 35.7±2.0
4 1 73073.252 -6.6 25.0±3.5 0.65±0.11 17.2±2.0
5 0 91342.732 -3.5 37.5±3.0 0.46±0.04 18.2±1.0
5 1 91340.865 14.2 11.9±3.0 0.49±0.11 6.3±1.0
6 0 109610.225 2.1 12.8±2.8 0.45±0.09 6.1±1.0
6 1 109607.954 -7.3 6.6±2.8 0.60±0.10 4.2±1.0

Notes.

a

Observed frequencies (in MHz) adopting a vLSR of 5.83 km s−1 for TMC-1. The uncertainty is 10 kHz for all the lines.

b

Observed minus calculated frequencies (in kHz) resulting from a fit to the observed frequencies. The J=7-6 K=0,1 lines observed in L1527 have been included in the fit (see text).

c

Antenna temperature (in mK).

d

Linewidth at half intensity (in kms−1). (e) Integrated line intensity (in mKkms−1).