Discovery of the elusive carbonic acid (HOCOOH) in space ...
After a quarter century since the detection of the last interstellar carboxylic acid, acetic acid (CH$_3$COOH), we report the discovery of a new one, the cis-trans form of carbonic acid (HOCOOH), toward the Galactic Center molecular cloud G+0.693-0.027. HOCOOH stands as the first interstellar molecu...
Main Authors: | , , , , , , , , , , , , , , |
---|---|
Format: | Text |
Language: | unknown |
Published: |
arXiv
2023
|
Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.2307.08644 https://arxiv.org/abs/2307.08644 |
id |
ftdatacite:10.48550/arxiv.2307.08644 |
---|---|
record_format |
openpolar |
spelling |
ftdatacite:10.48550/arxiv.2307.08644 2023-10-01T03:55:21+02:00 Discovery of the elusive carbonic acid (HOCOOH) in space ... Sanz-Novo, Miguel Rivilla, Víctor M. Jiménez-Serra, Izaskun Martín-Pintado, Jesús Colzi, Laura Zeng, Shaoshan Megías, Andrés López-Gallifa, Álvaro Martínez-Henares, Antonio Massalkhi, Sarah Tercero, Belén de Vicente, Pablo Martín, Sergio Andrés, David San Requena-Torres, Miguel A. 2023 https://dx.doi.org/10.48550/arxiv.2307.08644 https://arxiv.org/abs/2307.08644 unknown arXiv https://dx.doi.org/10.3847/1538-4357/ace523 Creative Commons Attribution Non Commercial No Derivatives 4.0 International https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode cc-by-nc-nd-4.0 Astrophysics of Galaxies astro-ph.GA FOS Physical sciences ScholarlyArticle Article article-journal Text 2023 ftdatacite https://doi.org/10.48550/arxiv.2307.0864410.3847/1538-4357/ace523 2023-09-04T14:46:06Z After a quarter century since the detection of the last interstellar carboxylic acid, acetic acid (CH$_3$COOH), we report the discovery of a new one, the cis-trans form of carbonic acid (HOCOOH), toward the Galactic Center molecular cloud G+0.693-0.027. HOCOOH stands as the first interstellar molecule containing three oxygen atoms and also the third carboxylic acid detected so far in the interstellar medium. Albeit the limited available laboratory measurements (up to 65 GHz), we have also identified several pairs of unblended lines directly in the astronomical data (between 75-120 GHz), which allowed us to slightly improve the set of spectroscopic constants. We derive a column density for cis-trans HOCOOH of $N$ = (6.4 $\pm$ 0.4) $\times$ 10$^{12}$ cm$^{-2}$, which yields an abundance with respect to molecular H$_2$ of 4.7 $\times$ 10$^{-11}$. Meanwhile, the extremely low dipole moment (about fifteen times lower) of the lower-energy conformer, cis-cis HOCOOH, precludes its detection. We obtain an upper limit ... : Accepted for publication in The Astrophysical Journal ... Text Carbonic acid DataCite Metadata Store (German National Library of Science and Technology) |
institution |
Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
topic |
Astrophysics of Galaxies astro-ph.GA FOS Physical sciences |
spellingShingle |
Astrophysics of Galaxies astro-ph.GA FOS Physical sciences Sanz-Novo, Miguel Rivilla, Víctor M. Jiménez-Serra, Izaskun Martín-Pintado, Jesús Colzi, Laura Zeng, Shaoshan Megías, Andrés López-Gallifa, Álvaro Martínez-Henares, Antonio Massalkhi, Sarah Tercero, Belén de Vicente, Pablo Martín, Sergio Andrés, David San Requena-Torres, Miguel A. Discovery of the elusive carbonic acid (HOCOOH) in space ... |
topic_facet |
Astrophysics of Galaxies astro-ph.GA FOS Physical sciences |
description |
After a quarter century since the detection of the last interstellar carboxylic acid, acetic acid (CH$_3$COOH), we report the discovery of a new one, the cis-trans form of carbonic acid (HOCOOH), toward the Galactic Center molecular cloud G+0.693-0.027. HOCOOH stands as the first interstellar molecule containing three oxygen atoms and also the third carboxylic acid detected so far in the interstellar medium. Albeit the limited available laboratory measurements (up to 65 GHz), we have also identified several pairs of unblended lines directly in the astronomical data (between 75-120 GHz), which allowed us to slightly improve the set of spectroscopic constants. We derive a column density for cis-trans HOCOOH of $N$ = (6.4 $\pm$ 0.4) $\times$ 10$^{12}$ cm$^{-2}$, which yields an abundance with respect to molecular H$_2$ of 4.7 $\times$ 10$^{-11}$. Meanwhile, the extremely low dipole moment (about fifteen times lower) of the lower-energy conformer, cis-cis HOCOOH, precludes its detection. We obtain an upper limit ... : Accepted for publication in The Astrophysical Journal ... |
format |
Text |
author |
Sanz-Novo, Miguel Rivilla, Víctor M. Jiménez-Serra, Izaskun Martín-Pintado, Jesús Colzi, Laura Zeng, Shaoshan Megías, Andrés López-Gallifa, Álvaro Martínez-Henares, Antonio Massalkhi, Sarah Tercero, Belén de Vicente, Pablo Martín, Sergio Andrés, David San Requena-Torres, Miguel A. |
author_facet |
Sanz-Novo, Miguel Rivilla, Víctor M. Jiménez-Serra, Izaskun Martín-Pintado, Jesús Colzi, Laura Zeng, Shaoshan Megías, Andrés López-Gallifa, Álvaro Martínez-Henares, Antonio Massalkhi, Sarah Tercero, Belén de Vicente, Pablo Martín, Sergio Andrés, David San Requena-Torres, Miguel A. |
author_sort |
Sanz-Novo, Miguel |
title |
Discovery of the elusive carbonic acid (HOCOOH) in space ... |
title_short |
Discovery of the elusive carbonic acid (HOCOOH) in space ... |
title_full |
Discovery of the elusive carbonic acid (HOCOOH) in space ... |
title_fullStr |
Discovery of the elusive carbonic acid (HOCOOH) in space ... |
title_full_unstemmed |
Discovery of the elusive carbonic acid (HOCOOH) in space ... |
title_sort |
discovery of the elusive carbonic acid (hocooh) in space ... |
publisher |
arXiv |
publishDate |
2023 |
url |
https://dx.doi.org/10.48550/arxiv.2307.08644 https://arxiv.org/abs/2307.08644 |
genre |
Carbonic acid |
genre_facet |
Carbonic acid |
op_relation |
https://dx.doi.org/10.3847/1538-4357/ace523 |
op_rights |
Creative Commons Attribution Non Commercial No Derivatives 4.0 International https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode cc-by-nc-nd-4.0 |
op_doi |
https://doi.org/10.48550/arxiv.2307.0864410.3847/1538-4357/ace523 |
_version_ |
1778523744857227264 |