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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. 3.

Fig. 3

Calculated fractional abundance of C5H4 (allowing for various isomers) as a function of time. The horizontal dashed line corresponds to the sum of the observed abundances of the two C5H4 isomers (CH3C4H and H2CCCHCCH) detected in TMC-1.