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...

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Main Authors: 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.
Format: Text
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Published: arXiv 2023
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Online Access:https://dx.doi.org/10.48550/arxiv.2307.08644
https://arxiv.org/abs/2307.08644
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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
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