Discovery of propenethial (CH

We present the detection of propenethial (CH2CHCHS), the sulphur analogue of interstellar acrolein (CH2CHCHO), towards TMC-1. The detection of this new sulphur molecule in TMC-1 is based on the data derived from rotational spectroscopy laboratory experiments, including new data in the millimetre wave domain, which are also presented in this work. Propenethial was observed in the cold dark cloud TMC-1 using data from the ongoing QUIJOTE line survey, which is being carried out with the Yebes 40m telescope. A total of nine rotational transitions with J = 6 up to 9 and Ka = 0 and 1 were detected in the 31.0–50.4 GHz range. We derive a total column density for propenethial of (4.4 ± 0.4) × 1010 cm−2, which is 2, 6.8, and 27 times smaller than those for CH3CHS, HCCHS, and NCCHS, which are the other thioaldehyde derivatives detected in TMC-1. The abundance ratio found in TMC-1 between the aldehyde counterpart, acrolein, and propenethial is 4.7, which is also different from those found for other pairs of aldehydes-thioaldehydes in this source. Our investigation of possible chemical formation pathways suggests that CH2CHCHS likely results from a combination of gas- and surface-phase reactions.

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2025-06-16
DOI
https://doi.org/10.1051/0004-6361/202554670/pdf
Primary Topic
Astrophysics and Star Formation Studies
Type
article
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article

Discovery of propenethial (CH

Springer Link (Chiba Institute of Technology)
Astrophysics and Star Formation Studies
article

Discovery of propenethial (CH

article en

Abstract

We present the detection of propenethial (CH2CHCHS), the sulphur analogue of interstellar acrolein (CH2CHCHO), towards TMC-1. The detection of this new sulphur molecule in TMC-1 is based on the data derived from rotational spectroscopy laboratory experiments, including new data in the millimetre wave domain, which are also presented in this work. Propenethial was observed in the cold dark cloud TMC-1 using data from the ongoing QUIJOTE line survey, which is being carried out with the Yebes 40m telescope. A total of nine rotational transitions with J = 6 up to 9 and Ka = 0 and 1 were detected in the 31.0–50.4 GHz range. We derive a total column density for propenethial of (4.4 ± 0.4) × 1010 cm−2, which is 2, 6.8, and 27 times smaller than those for CH3CHS, HCCHS, and NCCHS, which are the other thioaldehyde derivatives detected in TMC-1. The abundance ratio found in TMC-1 between the aldehyde counterpart, acrolein, and propenethial is 4.7, which is also different from those found for other pairs of aldehydes-thioaldehydes in this source. Our investigation of possible chemical formation pathways suggests that CH2CHCHS likely results from a combination of gas- and surface-phase reactions.

Springer Link (Chiba Institute of Technology)
Openalex Percentile: Top 64%
Astrophysics and Star Formation Studies
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