Search Results - "Esplugues, G"
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1
Dust temperature and time-dependent effects in the chemistry of photodissociation regions
Published in Monthly notices of the Royal Astronomical Society (12-04-2019)Get full text
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2
Parameterizing the interstellar dust temperature
Published 16-04-2017“…A&A 604, A58 (2017) The temperature of interstellar dust particles is of great importance to astronomers. It plays a crucial role in the thermodynamics of…”
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3
Surface chemistry in photodissociation regions
Published 22-04-2016“…The presence of dust can strongly affect the chemical composition of the interstellar medium. We model the chemistry in photodissociation regions (PDRs) using…”
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4
Modelling the sulphur chemistry evolution in Orion KL
Published 09-06-2014“…We study the sulphur chemistry evolution in the Orion KL along the gas and grain phases of the cloud. We investigate the processes that dominate the sulphur…”
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5
Extended warm gas in Orion KL as probed by methyl cyanide
Published 12-02-2014“…In order to study the temperature distribution of the extended gas within the Orion Kleinmann-Low nebula, we have mapped the emission by methyl cyanide (CH3CN)…”
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6
A line confusion-limited millimeter survey of Orion KL. III. Sulfur oxide species
Published 23-06-2013“…We present a study of the sulfur-bearing species detected in a line confusion-limited survey towards Orion KL performed with the IRAM 30m telescope in the…”
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7
A combined IRAM and Herschel/HIFI study of cyano(di)acetylene in Orion KL: tentative detection of DC3N
Published 02-09-2013“…We present a study of cyanoacetylene (HC3N) and cyanodiacetylene (HC5N) in Orion KL, through observations from two line surveys performed with the IRAM 30m…”
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Evolution of Chemistry in the envelope of HOt CorinoS (ECHOS) II. The puzzling chemistry of isomers as revealed by the HNCS/HSCN ratio
Published 08-11-2024“…The observational detection of some metastable isomers in the interstellar medium with abundances comparable to those of the most stable isomer, or even when…”
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Gas phase Elemental abundances in Molecular cloudS (GEMS). X. Observational effects of turbulence on the chemistry of molecular clouds
Published 05-10-2024“…Astronomy & Astrophysics 2024, Volume 688, id.A188, 17 pp (Abridged) We explore the chemistry of the most abundant C, O, S, and N bearing species in molecular…”
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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 B335
Published 04-09-2023“…A&A 678, A199 (2023) Within the project Evolution of Chemistry in the envelope of HOt corinoS (ECHOS), we present a study of sulphur chemistry in the envelope…”
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11
H2CS deuteration maps towards the pre-stellar core L1544
Published 15-03-2022“…A&A 661, A111 (2022) Deuteration is a crucial tool to understand the complexity of interstellar chemical processes, especially when they involve the interplay…”
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Gas phase Elemental abundances in Molecular cloudS (GEMS) VI. A sulphur journey across star-forming regions: study of thioformaldehyde emission
Published 06-04-2022“…In the context of the IRAM 30m Large Program GEMS, we present a study of thioformaldehyde in several starless cores located in star-forming filaments of…”
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13
Linking the dust and chemical evolution: Taurus and Perseus -- New collisional rates for HCN, HNC, and their C, N, and H isotopologues
Published 15-12-2022“…A&A 670, A110 (2023) HCN, HNC, and their isotopologues are ubiquitous molecules that can serve as chemical thermometers and evolutionary tracers to…”
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Gas phase Elemental abundances in Molecular cloudS (GEMS) VII. Sulfur elemental abundance
Published 07-12-2022“…A&A 670, A114 (2023) Gas phase Elemental abundances in molecular CloudS (GEMS) is an IRAM 30m large program aimed at determining the elemental abundances of…”
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Gas phase Elemental abundances in Molecular cloudS (GEMS). IV. Observational results and statistical trends
Published 25-02-2021“…A&A 648, A120 (2021) Gas phase Elemental abundances in Molecular CloudS (GEMS) is an IRAM 30m Large Program designed to estimate the S, C, N, and O depletions…”
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Gas-phase Elemental abundances in Molecular cloudS (GEMS) III. Unlocking the CS chemistry: the CS+O reaction
Published 18-12-2020“…Astronomy & Astrophysics 646, A5 (2021) CS is among the most abundant gas-phase S-bearing molecules in cold dark molecular clouds. It is easily observable with…”
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