2022A&A...663L...9C


Query : 2022A&A...663L...9C

2022A&A...663L...9C - Astronomy and Astrophysics, volume 663L9-9 (2022/7-1)

Discovery of fulvenallene in TMC-1 with the QUIJOTE line survey.

CERNICHARO J., FUENTETAJA R., AGUNDEZ M., KAISER R.I., CABEZAS C., MARCELINO N., TERCERO B., PARDO J.R. and DE VICENTE P.

Abstract (from CDS):

We report the detection of fulvenallene (c-C5H4CCH2) in the direction of TMC-1 with the QUIJOTE1 line survey. Thirty rotational transitions with Ka = 0,1,2,3 and J = 9-15 were detected. The best rotational temperature fitting of the data is 9 K and a derived column density is (2.7 ± 0.3) x 1012 cm–2, which is only a factor of 4.4 below that of its potential precursor cyclopentadiene (c-C5H6), and 1.4-1.9 times higher than that of the ethynyl derivatives of cyclopentadiene. We searched for fulvene (c-C5H4CH2), a CH2 derivative of cyclopentadiene, for which we derive a 3σ upper limit to its column density of (3.5 ± 0.5) x 1012 cm–2. Upper limits were also obtained for toluene (C6H5CH3) and styrene (C6H5C2H3), the methyl and vinyl derivatives of benzene. Fulvenallene and ethynyl cyclopentadiene are likely formed in the reaction between cyclopentadiene (c-C5H6) and the ehtynyl radical (CCH). However, the bottom-up gas-phase synthesis of cycles in TMC-1 underestimates the abundance of cyclopentadiene by two orders of magnitude, which strengthens the need to study all possible chemical pathways to cyclisation in cold dark cloud environments, such as TMC-1. However, the inclusion of the reaction between C3H3 and C2H4 produces a good agreement between model and observed abundances.

Abstract Copyright: © J. Cernicharo et al. 2022

Journal keyword(s): molecular data - line: identification - ISM: molecules - ISM: individual objects: TMC-1 - astrochemistry

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
2 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0

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