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Sökning: WFRF:(Godard A.) > Detection of hydrog...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00007768naa a2201045 4500
001oai:research.chalmers.se:fac96824-3166-481c-abd5-c64f4bfe40b6
003SwePub
008171007s2010 | |||||||||||000 ||eng|
024a https://doi.org/10.1051/0004-6361/2010150822 DOI
024a https://research.chalmers.se/publication/1318452 URI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Sonnentrucker, P.u Johns Hopkins University4 aut
2451 0a Detection of hydrogen fluoride absorption in diffuse molecular clouds with Herschel/HIFI: an ubiquitous tracer of molecular gas
264 c 2010-10-01
264 1b EDP Sciences,c 2010
338 a electronic2 rdacarrier
520 a We discuss the detection of absorption by interstellar hydrogen fluoride (HF) along the sight line to the submillimeter continuum sources W49N and W51. We have used Herschel's HIFI instrument in dual beam switch mode to observe the 1232.4762 GHz J = 1-0 HF transition in the upper sideband of the band 5a receiver. We detected foreground absorption by HF toward both sources over a wide range of velocities. Optically thin absorption components were detected on both sight lines, allowing us to measure - as opposed to obtain a lower limit on - the column density of HF for the first time. As in previous observations of HF toward the source G10.6-0.4, the derived HF column density is typically comparable to that of water vapor, even though the elemental abundance of oxygen is greater than that of fluorine by four orders of magnitude. We used the rather uncertain N(CH) - N(H-2) relationship derived previously toward diffuse molecular clouds to infer the molecular hydrogen column density in the clouds exhibiting HF absorption. Within the uncertainties, we find that the abundance of HF with respect to H-2 is consistent with the theoretical prediction that HF is the main reservoir of gas-phase fluorine for these clouds. Thus, hydrogen fluoride has the potential to become an excellent tracer of molecular hydrogen, and provides a sensitive probe of clouds of small H-2 column density. Indeed, the observations of hydrogen fluoride reported here reveal the presence of a low column density diffuse molecular cloud along the W51 sight line, at an LSR velocity of similar to 24 km s(-1), that had not been identified in molecular absorption line studies prior to the launch of Herschel.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a submillimeter: ISM
653 a w49n
653 a ISM: molecules
653 a h2o
653 a regions
653 a abundance
653 a astronomy
653 a line-of-sight
653 a astrochemistry
653 a w51
653 a molecular processes
653 a co
700a Neufeld, D. A.u Johns Hopkins University4 aut
700a Phillips, T. G.u California Institute of Technology (Caltech)4 aut
700a Gerin, M.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Lis, D. C.u California Institute of Technology (Caltech)4 aut
700a de Luca, M.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Goicoechea, J. R.u Centro de Astrobiologia (CAB)4 aut
700a Black, John H,d 1949u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)jblack
700a Bell, T. A.u California Institute of Technology (Caltech)4 aut
700a Boulanger, F.u Institut d'Astrophysique Spatiale4 aut
700a Cernicharo, J.u Centro de Astrobiologia (CAB)4 aut
700a Coutens, A.u Université de Toulouse,University of Toulouse4 aut
700a Dartois, E.u Institut d'Astrophysique Spatiale4 aut
700a Kazmierczak, M.u Uniwersytet Mikolaja Kopernika w Toruniu,Nicolaus Copernicus University4 aut
700a Encrenaz, P.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Falgarone, E.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Geballe, T. R.u Gemini Observatory North4 aut
700a Giesen, T.u Universität zu Köln,University of Cologne4 aut
700a Godard, B.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Goldsmith, P. F.4 aut
700a Gry, C.u Laboratoire d'Astrophysique de Marseille4 aut
700a Gupta, H.4 aut
700a Hennebelle, P.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Herbst, E.u Ohio State University4 aut
700a Hily-Blant, P.4 aut
700a Joblin, C.u Université de Toulouse,University of Toulouse4 aut
700a Kolos, R.u Polish Academy of Sciences4 aut
700a Krelowski, J.u Uniwersytet Mikolaja Kopernika w Toruniu,Nicolaus Copernicus University4 aut
700a Martin-Pintado, J.u Centro de Astrobiologia (CAB)4 aut
700a Menten, K. M.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Monje, Raquel,d 1979u California Institute of Technology (Caltech)4 aut0 (Swepub:cth)em1raque
700a Mookerjea, B.u Tata Institute of Fundamental Research4 aut
700a Pearson, J. C.4 aut
700a Perault, M.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Persson, Carina,d 1964u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)carina64
700a Plume, R.u University of Calgary4 aut
700a Salez, M.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Schlemmer, S.u Universität zu Köln,University of Cologne4 aut
700a Schmidt, M.u Polish Academy of Sciences4 aut
700a Stutzki, J.u Universität zu Köln,University of Cologne4 aut
700a Teyssier, D.u European Space Astronomy Centre (ESAC)4 aut
700a Vastel, C.u Université de Toulouse,University of Toulouse4 aut
700a Yu, S.4 aut
700a Caux, E.u Université de Toulouse,University of Toulouse4 aut
700a Güsten, R.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Hatch, W. A.4 aut
700a Klein, T.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Mehdi, Imran4 aut
700a Morris, P.u California Institute of Technology (Caltech)4 aut
700a Ward, J. S.4 aut
710a Johns Hopkins Universityb California Institute of Technology (Caltech)4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 521:1, s. Article Number: L12-q 521:1<Article Number: L12-x 0004-6361x 1432-0746
856u http://publications.lib.chalmers.se/records/fulltext/local_131845.pdfx primaryx freey FULLTEXT
856u https://www.aanda.org/articles/aa/pdf/2010/13/aa15082-10.pdf
8564 8u https://doi.org/10.1051/0004-6361/201015082
8564 8u https://research.chalmers.se/publication/131845

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