Discovery of CH2CCHC4H and a rigorous detection of CH2CCHC3N in TMC-1 with the QUIJOTE line survey
arXiv:2206.08992 · doi:10.1051/0004-6361/202243857
Abstract
Using the QUIJOTE line survey in the 32.0-50.4 GHz range, we report the discovery of the molecule CH2CCHC4H towards the prestellar cold core TMC-1 in the Taurus region. We also present a rigorous detection of CH2CCHC3N, along with its detailed analysis. We identified a total of twenty rotational transitions for each one of these molecules. The rotational quantum numbers range from Ju=17 up to 24 and Ka<=3. The column density for CH2CCHC4H is N=(2.2+/-0.2)x 1E12 cm-2, while for CH2CCHC3N, we derived N=(1.2+/-0.15) x 1E11 cm-2. The rotational temperature is 9.0+/-0.5 K for both species. The abundance ratio between CH2CCHC4H and CH2CCHC3N is 18+/-4. We also compared the column densities of these species with those of their isomers CH3C6H and CH3C5N, derived from their J=20-19 up to J=30-29 rotational transitions observed with the QUIJOTE line survey. The observed abundances for all these species are reasonably well explained by state-of-the-art chemical models of TMC-1. The observed astronomical frequencies were merged with laboratory frequencies from the literature to derive improved spectroscopic parameters.
Astronomy and Astrophysics, in press. arXiv admin note: text overlap with arXiv:2112.01130
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Cited by in corpus (7)
- Discovery of fulvenallene in TMC-1 with the QUIJOTE line survey
- Discovery of two cyano derivatives of acenaphthylene (CH) in TMC-1 with the QUIJOTE line survey
- Carbon-Chain Chemistry in the Interstellar Medium
- Discovery of two new interstellar molecules with QUIJOTE: HCCCHCCC and HCCCCS
- Laboratory and astronomical discovery of cyanothioketene, NCCHCS, in the cold starless core TMC-1
- Discovery of CH3CHCO in TMC-1 with the QUIJOTE line survey
- Chemistry of Dark Molecular Clouds