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 2. Derived spectroscopic parameters (in MHz) for CH3CO+.

Constant Spacea Laboratoryb Mergedc
B 9134.47424(82) 9134.47083(27) 9134.47211(20)
DJ 4.014(12) 10−3 3.99198(25) 10−3 3.99307(21) 10−3
DJK 1.8847(53)10−1 1.87616(41) 10−1 1.87736(46) 10−1
HJK 8.66(33) 10−7 9.56(37) 10−7
HKJ 6.58(59) 10−6 7.19(74) 10−6
rms(kHz)d 6.9 34.3 33.2
Jmin/Jmax 1/7 10/27 1 /27
Kmin/Kmax 0/1 0/6 0/6
Nlines e 10 79 89
νmax(GHz) 127.87 492.95 492.95

Notes.

a

Fit to the lines of CH3CO+ observed in TMC-1. In this fit, the J=7-6 and K=0,1 lines observed in L1527 (with frequencies of 127877.133±0.025 and 127874.494±0.050 MHz, respectively) have been included (see Fig. A.1 and Appendix A).

b

Fit to the lines of CH3CO+ observed in the laboratory.

c

Fit to the the lines of CH3CO+ observed in space and in the laboratory.

d

The standard deviation of the fit (in kHz). (e) Number of lines included in the fit.