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dc.contributor.authorANDERSON, Dana E.
dc.contributor.authorBERGIN, Edwin A.
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG ]
dc.contributor.authorMARET, Sébastien
hal.structure.identifierAMOR 2013
dc.contributor.authorWAKELAM, Valentine
dc.date.issued2013-12
dc.identifier.issn0004-637X
dc.description.abstractEnWe present observations of fine-structure line emission of atomic sulfur, iron, and rotational lines of molecular hydrogen in shocks associated with several Class 0 protostars obtained with the Infrared Spectrograph of the Spitzer Space Telescope. We use these observations to investigate the "missing sulfur problem," that significantly less sulfur is found in dense regions of the interstellar medium (ISM) than in diffuse regions. For sources where the sulfur fine-structure line emission is co-spatial with the detected molecular hydrogen emission and in the presence of weak iron emission, we derive sulfur and H2 column densities for the associated molecule-dominated C-shocks. We find the S I abundance to be gsim5%-10% of the cosmic sulfur abundance, indicating that atomic sulfur is a major reservoir of sulfur in shocked gas. This result suggests that in the quiescent dense ISM sulfur is present in some form that is released from grains as atoms, perhaps via sputtering, within the shock.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.enastrochemistry
dc.subject.enISM: abundances
dc.subject.enISM: atoms
dc.subject.enISM: molecules
dc.title.enNew Constraints on the Sulfur Reservoir in the Dense Interstellar Medium Provided by Spitzer Observations of S I in Shocked Gas
dc.typeArticle de revue
dc.identifier.doi10.1088/0004-637X/779/2/141
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
bordeaux.journalThe Astrophysical Journal
bordeaux.page141
bordeaux.volume779
bordeaux.peerReviewedoui
hal.identifierhal-00949933
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00949933v1
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