dc.contributor.author | NEUFELD, D. A. | |
dc.contributor.author | SONNENTRUCKER, P. | |
hal.structure.identifier | California Institute of Technology [CALTECH] | |
dc.contributor.author | PHILLIPS, T. G. | |
hal.structure.identifier | California Institute of Technology [CALTECH] | |
dc.contributor.author | LIS, D. C. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | DE LUCA, M. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | GOICOECHEA, J. R. | |
dc.contributor.author | BLACK, J. H. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
hal.structure.identifier | Laboratoire de Radioastronomie [LRA] | |
dc.contributor.author | GERIN, M. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Grenoble [LAOG] | |
dc.contributor.author | BELL, T. | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | BOULANGER, F. | |
hal.structure.identifier | Centro de Investigaciones Biológicas [CSIC] | |
dc.contributor.author | CERNICHARO, J. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Grenoble [LAOG] | |
dc.contributor.author | COUTENS, A. | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | DARTOIS, E. | |
dc.contributor.author | KAZMIERCZAK, M. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | ENCRENAZ, P. | |
hal.structure.identifier | Laboratoire de Radioastronomie [LRA] | |
dc.contributor.author | FALGARONE, E. | |
dc.contributor.author | GEBALLE, T. R. | |
dc.contributor.author | GIESEN, T. | |
dc.contributor.author | GODARD, B. | |
dc.contributor.author | GOLDSMITH, P. F. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | GRY, C. | |
hal.structure.identifier | Indian Institute of Technology Delhi [IIT Delhi] | |
dc.contributor.author | GUPTA, H. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Grenoble [LAOG] | |
dc.contributor.author | HENNEBELLE, P. | |
hal.structure.identifier | The Ohio State University [Columbus] [OSU] | |
dc.contributor.author | HERBST, E. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Grenoble [LAOG] | |
dc.contributor.author | HILY-BLANT, Pierre | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | JOBLIN, C. | |
dc.contributor.author | KOLOS, R. | |
dc.contributor.author | KRELOWSKI, J. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Grenoble [LAOG] | |
dc.contributor.author | MARTIN-PINTADO, J. | |
hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
dc.contributor.author | MENTEN, K. M. | |
dc.contributor.author | MONJE, R. | |
hal.structure.identifier | KOSMA, I. Physikalisches Institut | |
dc.contributor.author | MOOKERJEA, B. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Grenoble [LAOG] | |
dc.contributor.author | PEARSON, Justin | |
hal.structure.identifier | Laboratoire de Radioastronomie [LRA] | |
dc.contributor.author | PERAULT, M. | |
hal.structure.identifier | Department of Materials Science and Engineering, KTH [KTH] | |
dc.contributor.author | PERSSON, C. | |
dc.contributor.author | PLUME, R. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Grenoble [LAOG] | |
dc.contributor.author | SALEZ, M. | |
dc.contributor.author | SCHLEMMER, S. | |
hal.structure.identifier | Department of Obstetrics and Gynecology | |
dc.contributor.author | SCHMIDT, M. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Grenoble [LAOG] | |
dc.contributor.author | STUTZKI, J. | |
hal.structure.identifier | Herschel Science Center [Madrid] | |
dc.contributor.author | TEYSSIER, D. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | VASTEL, C. | |
dc.contributor.author | YU, S. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
hal.structure.identifier | Observatoire aquitain des sciences de l'univers [OASU] | |
hal.structure.identifier | Université Sciences et Technologies - Bordeaux 1 [UB] | |
hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
dc.contributor.author | CAIS, Ph. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | CAUX, E. | |
dc.contributor.author | LISEAU, R. | |
dc.contributor.author | MORRIS, P. | |
dc.contributor.author | PLANESAS, P. | |
dc.date.created | 2010 | |
dc.date.issued | 2010 | |
dc.identifier.issn | 0004-6361 | |
dc.description.abstractEn | We report the detection of strong absorption by interstellar hydrogen fluoride along the sight-line to the submillimeter continuum source G10.6-0.4 (W31C). We have used Herschel's HIFI instrument, in dual beam switch mode, to observe the 1232.4763 GHz J=1-0 HF transition in the upper sideband of the Band 5a receiver. The resultant spectrum shows weak HF emission from G10.6-0.4 at LSR velocities in the range -10 to -3 km/s, accompanied by strong absorption by foreground material at LSR velocities in the range 15 to 50 km/s. The spectrum is similar to that of the 1113.3430 GHz 1(11)-0(00) transition of para-water, although at some frequencies the HF (hydrogen fluoride) optical depth clearly exceeds that of para-H2O. The optically-thick HF absorption that we have observed places a conservative lower limit of 1.6E+14 cm-2 on the HF column density along the sight-line to G10.6-0.4. Our lower limit on the HF abundance, 6E-9 relative to hydrogen nuclei, implies that hydrogen fluoride accounts for between ~ 30 and 100% of the fluorine nuclei in the gas phase along this sight-line. This observation corroborates theoretical predictions that - because the unique thermochemistry of fluorine permits the exothermic reaction of F atoms with molecular hydrogen - HF will be the dominant reservoir of interstellar fluorine under a wide range of conditions. | |
dc.language.iso | en | |
dc.publisher | EDP Sciences | |
dc.subject.en | ISM: molecules | |
dc.subject.en | submillimeter: ISM | |
dc.subject.en | molecular processes | |
dc.title.en | Strong absorption by interstellar hydrogen fluoride: Herschel/HIFI observations of the sight-line to G10.6-0.4 (W31C) | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1051/0004-6361/201014523 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
dc.identifier.arxiv | 1005.1671 | |
bordeaux.journal | Astronomy and Astrophysics - A&A | |
bordeaux.page | L108 | |
bordeaux.volume | 518 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00521637 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00521637v1 | |
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