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hal.structure.identifierObservatorio Astronomico Nacional, Madrid
dc.contributor.authorFUENTE, Asuncion
hal.structure.identifierConsejo Superior de Investigaciones Cientificas [España] = Spanish National Research Council [Spain] [CSIC]
dc.contributor.authorGOICOECHEA, Javier
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorPETY, Jérôme
dc.contributor.authorLE GAL, Romane
dc.contributor.authorMARTÍN-DOMÉNECH, Rafael
hal.structure.identifierAMOR 2017
dc.contributor.authorGRATIER, P.
hal.structure.identifierJoint ALMA Observatory [JAO]
dc.contributor.authorGUZMAN, Viviana
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorROUEFF, Evelyne
hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorLOISON, Jean Christophe
dc.contributor.authorMUÑOZ-CARO, Guillermo M.
hal.structure.identifierAMOR 2017
dc.contributor.authorWAKELAM, Valentine
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorGERIN, Maryvonne
hal.structure.identifierEuropean Space Astronomy Centre [ESAC]
dc.contributor.authorRIVIERE-MARICHALAR, Pablo
hal.structure.identifierAMOR 2017
dc.contributor.authorVIDAL, Thomas
dc.date.issued2017
dc.identifier.issn2041-8205
dc.description.abstractEnWe present the first detection of gas phase S2H in the Horsehead, a moderately UV-irradiated nebula. This confirms the presence of doubly sulfuretted species in the interstellar medium and opens a new challenge for sulfur chemistry. The observed S2H abundance is ~5x10$^{-11}$, only a factor 4-6 lower than that of the widespread H2S molecule. H2S and S2H are efficiently formed on the UV-irradiated icy grain mantles. We performed ice irradiation experiments to determine the H2S and S2H photodesorption yields. The obtained values are ~1.2x10$^{-3}$ and <1x10$^{-5}$ molecules per incident photon for H2S and S2H, respectively. Our upper limit to the S2H photodesorption yield suggests that photo-desorption is not a competitive mechanism to release the S2H molecules to the gas phase. Other desorption mechanisms such as chemical desorption, cosmic-ray desorption and grain shattering can increase the gaseous S2H abundance to some extent. Alternatively, S2H can be formed via gas phase reactions involving gaseous H2S and the abundant ions S+ and SH+. The detection of S2H in this nebula could be therefore the result of the coexistence of an active grain surface chemistry and gaseous photo-chemistry.
dc.language.isoen
dc.publisherBristol : IOP Publishing
dc.subject.enAstrochemistry
dc.subject.enmethods: laboratory: solid state
dc.subject.enISM: abundances
dc.subject.enISM: molecules
dc.subject.enphotondominated region (PDR)
dc.subject.enHorsehead
dc.title.enFirst detection of interstellar S2H
dc.typeArticle de revue
dc.identifier.doi10.3847/2041-8213/aaa01b
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
dc.identifier.arxiv1712.03036
bordeaux.journalThe Astrophysical journal letters
bordeaux.pageL49
bordeaux.volume851
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-01661652
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01661652v1
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