Discovery of H2CCCH+ in TMC-1 (Corrigendum)

W. G. D. P. Silva,J. Cernicharo, S. Schlemmer,N. Marcelino,J. -c. Loison, M. Agundez, D. Gupta, V. Wakelam,S. Thorwirth, C. Cabezas, B. Tercero, J. L. Domenech, R. Fuentetaja, W. -j. Kim,P. de Vicente,O. Asvany

ASTRONOMY & ASTROPHYSICS(2023)

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摘要
Based on a novel laboratory method, 14 millimeter-wave lines of the molecular ion H2CCCH+ have been measured in high resolution, and the spectroscopic constants of this asymmetric rotor determined with high accuracy. Using the Yebes 40 m and IRAM 30 m radio telescopes, we detected four lines of H2CCCH+ toward the cold dense core TMC-1. With a dipole moment of about 0.55 D obtained from high-level ab initio calculations, we derive a column density of 5.4 & PLUSMN;1x10(11) cm(-2) and 1.6 & PLUSMN;0.5x10(11) cm(-2) for the ortho and para species, respectively, and an abundance ratio N(H2CCC)/N(H2CCCH+) = 2.8 & PLUSMN;0.7. The chemistry of H2CCCH+ is modeled using the most recent chemical network for the reactions involving the formation of H2CCCH+. We find a reasonable agreement between model predictions and observations, and new insights into the chemistry of C-3-bearing species in TMC-1 were obtained.
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关键词
astrochemistry, ISM: molecules, ISM: individual objects: TMC-1, methods: laboratory: molecular, molecular data, errata, addenda
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