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. Author manuscript; available in PMC: 2021 Apr 12.
Published in final edited form as: Astron Astrophys. 2021 Mar 11;647:L3. doi: 10.1051/0004-6361/202140482

Fig. 2.

Fig. 2

Observed transitions of CH3C4H towards TMC-1. The abscissa corresponds to the rest frequency of the lines assuming a local standard of rest velocity of TMC-1 of 5.83 km s–1. Line parameters for the observed transitions are given in Table A.1. The ordinate is the antenna temperature, corrected for atmospheric and telescope losses, in millikelvin. The red line shows the computed synthetic spectrum for this species for Tr=7 K and a column density of 6.5×1012 cm–2 for each of the A and E states of vinyl diacetylene.