Asunción Fuente

Employment

• Centro de Astrobiología
  2023 - Present

Education

Education history is unavailable.

Projects & Funding

Projects & funding information is unavailable.

Publications (263)

• Evolution of Chemistry in the envelope of HOt corinoS (ECHOS): I. Extremely young sulphur chemistry in the isolated Class 0 object B 335
  Astronomy and Astrophysics 2023 DOI: 10.1051/0004-6361/202346721
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• Evolution of Chemistry in the envelope of Hot Corinos (ECHOS) I. Extremely young sulphur chemistry in the isolated Class 0 object B 335
  arXiv 2023 DOI: 10.48550/arXiv.2309.01713
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• Formation of the methyl cation by photochemistry in a protoplanetary disk
  Olivier Berné, Marie‐Aline Martin‐Drumel, Ilane Schroetter +53 more
  Nature 2023 DOI: 10.1038/s41586-023-06307-x
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• Gas phase Elemental abundances in Molecular cloudS (GEMS) IX. Deuterated compounds of H2S in starless cores
  arXiv 2023 DOI: 10.48550/arXiv.2309.00318
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• Gas phase Elemental abundances in Molecular cloudS (GEMS) VIII. Unlocking the CS chemistry: the CH + S→ CS + H and C2 + S→ CS + C reactions
  arXiv 2023
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• Gas phase Elemental abundances in Molecular cloudS (GEMS): VII. Sulfur elemental abundance
  Astronomy and Astrophysics 2023 DOI: 10.1051/0004-6361/202244843
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• Gas phase Elemental abundances in Molecular cloudS (GEMS): VIII. Unlocking the CS chemistry: The CH + S → CS + H and C2 + S → CS + C reactions
  Astronomy and Astrophysics 2023 DOI: 10.1051/0004-6361/202346967
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• Linking the dust and chemical evolution: Taurus and Perseus: New collisional rates for HCN, HNC, and their C, N, and H isotopologues
  Astronomy and Astrophysics 2023 DOI: 10.1051/0004-6361/202245000
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• NIKA2 observations of starless cores in Taurus and Perseus
  arXiv 2023 DOI: 10.48550/arXiv.2310.01044
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• PDRs4All II: JWST’s NIR and MIR imaging view of the Orion Nebula
  arXiv 2023 DOI: 10.48550/arXiv.2308.16732
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• PDRs4All III: JWST’s NIR spectroscopic view of the Orion Bar
  arXiv 2023 DOI: 10.48550/arXiv.2310.08720
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• PDRs4All IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar
  arXiv 2023 DOI: 10.48550/arXiv.2308.16733
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• PRODIGE envelope to disk with NOEMA: II. Small-scale temperature structure and streamer feeding the SVS13A protobinary based on CH3CN and DCN
  Astronomy and Astrophysics 2023 DOI: 10.1051/0004-6361/202244183
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• AB Aur, a Rosetta stone for studies of planet formation (II): H2S detection and sulfur budget
  arXiv 2022 DOI: 10.48550/arXiv.2207.06716
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• AB Aur, a Rosetta stone for studies of planet formation: II. H2S detection and sulfur budget
  Astronomy and Astrophysics 2022 DOI: 10.1051/0004-6361/202142906
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• Gas phase Elemental abundances in Molecular cloudS (GEMS) V. Methanol in Taurus
  Astronomy and Astrophysics 2022 DOI: 10.1051/0004-6361/202141971
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• Gas phase Elemental abundances in Molecular cloudS (GEMS) VI. A sulphur journey across star-forming regions: study of thioformaldehyde emission
  arXiv 2022 DOI: 10.48550/arxiv.2204.02645
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• Gas phase Elemental abundances in Molecular cloudS (GEMS) VII. Sulfur elemental abundance
  arXiv 2022 DOI: 10.48550/arXiv.2212.03742
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• Gas phase Elemental abundances in Molecular cloudS (GEMS): VI. A sulphur journey across star-forming regions: study of thioformaldehyde emission
  Astronomy and Astrophysics 2022 DOI: 10.1051/0004-6361/202142936
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• H2CS deuteration maps towards the pre-stellar core L1544
  Astronomy and Astrophysics 2022 DOI: 10.1051/0004-6361/202243073
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