Sökning: WFRF:(Godard A.) > Detection of hydrog...
Fältnamn | Indikatorer | Metadata |
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000 | 07768naa a2201045 4500 | |
001 | oai:research.chalmers.se:fac96824-3166-481c-abd5-c64f4bfe40b6 | |
003 | SwePub | |
008 | 171007s2010 | |||||||||||000 ||eng| | |
024 | 7 | a https://doi.org/10.1051/0004-6361/2010150822 DOI |
024 | 7 | a https://research.chalmers.se/publication/1318452 URI |
040 | a (SwePub)cth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a art2 swepub-publicationtype |
072 | 7 | a ref2 swepub-contenttype |
100 | 1 | a Sonnentrucker, P.u Johns Hopkins University4 aut |
245 | 1 0 | a Detection of hydrogen fluoride absorption in diffuse molecular clouds with Herschel/HIFI: an ubiquitous tracer of molecular gas |
264 | c 2010-10-01 | |
264 | 1 | b 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 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a 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 | |
700 | 1 | a Neufeld, D. A.u Johns Hopkins University4 aut |
700 | 1 | a Phillips, T. G.u California Institute of Technology (Caltech)4 aut |
700 | 1 | a Gerin, M.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut |
700 | 1 | a Lis, D. C.u California Institute of Technology (Caltech)4 aut |
700 | 1 | a de Luca, M.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut |
700 | 1 | a Goicoechea, J. R.u Centro de Astrobiologia (CAB)4 aut |
700 | 1 | a Black, John H,d 1949u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)jblack |
700 | 1 | a Bell, T. A.u California Institute of Technology (Caltech)4 aut |
700 | 1 | a Boulanger, F.u Institut d'Astrophysique Spatiale4 aut |
700 | 1 | a Cernicharo, J.u Centro de Astrobiologia (CAB)4 aut |
700 | 1 | a Coutens, A.u Université de Toulouse,University of Toulouse4 aut |
700 | 1 | a Dartois, E.u Institut d'Astrophysique Spatiale4 aut |
700 | 1 | a Kazmierczak, M.u Uniwersytet Mikolaja Kopernika w Toruniu,Nicolaus Copernicus University4 aut |
700 | 1 | a Encrenaz, P.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut |
700 | 1 | a Falgarone, E.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut |
700 | 1 | a Geballe, T. R.u Gemini Observatory North4 aut |
700 | 1 | a Giesen, T.u Universität zu Köln,University of Cologne4 aut |
700 | 1 | a Godard, B.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut |
700 | 1 | a Goldsmith, P. F.4 aut |
700 | 1 | a Gry, C.u Laboratoire d'Astrophysique de Marseille4 aut |
700 | 1 | a Gupta, H.4 aut |
700 | 1 | a Hennebelle, P.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut |
700 | 1 | a Herbst, E.u Ohio State University4 aut |
700 | 1 | a Hily-Blant, P.4 aut |
700 | 1 | a Joblin, C.u Université de Toulouse,University of Toulouse4 aut |
700 | 1 | a Kolos, R.u Polish Academy of Sciences4 aut |
700 | 1 | a Krelowski, J.u Uniwersytet Mikolaja Kopernika w Toruniu,Nicolaus Copernicus University4 aut |
700 | 1 | a Martin-Pintado, J.u Centro de Astrobiologia (CAB)4 aut |
700 | 1 | a 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 |
700 | 1 | a Monje, Raquel,d 1979u California Institute of Technology (Caltech)4 aut0 (Swepub:cth)em1raque |
700 | 1 | a Mookerjea, B.u Tata Institute of Fundamental Research4 aut |
700 | 1 | a Pearson, J. C.4 aut |
700 | 1 | a Perault, M.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut |
700 | 1 | a Persson, Carina,d 1964u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)carina64 |
700 | 1 | a Plume, R.u University of Calgary4 aut |
700 | 1 | a Salez, M.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut |
700 | 1 | a Schlemmer, S.u Universität zu Köln,University of Cologne4 aut |
700 | 1 | a Schmidt, M.u Polish Academy of Sciences4 aut |
700 | 1 | a Stutzki, J.u Universität zu Köln,University of Cologne4 aut |
700 | 1 | a Teyssier, D.u European Space Astronomy Centre (ESAC)4 aut |
700 | 1 | a Vastel, C.u Université de Toulouse,University of Toulouse4 aut |
700 | 1 | a Yu, S.4 aut |
700 | 1 | a Caux, E.u Université de Toulouse,University of Toulouse4 aut |
700 | 1 | a Güsten, R.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
700 | 1 | a Hatch, W. A.4 aut |
700 | 1 | a Klein, T.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
700 | 1 | a Mehdi, Imran4 aut |
700 | 1 | a Morris, P.u California Institute of Technology (Caltech)4 aut |
700 | 1 | a Ward, J. S.4 aut |
710 | 2 | a Johns Hopkins Universityb California Institute of Technology (Caltech)4 org |
773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 521:1, s. Article Number: L12-q 521:1<Article Number: L12-x 0004-6361x 1432-0746 |
856 | 4 | u http://publications.lib.chalmers.se/records/fulltext/local_131845.pdfx primaryx freey FULLTEXT |
856 | 4 | u https://www.aanda.org/articles/aa/pdf/2010/13/aa15082-10.pdf |
856 | 4 8 | u https://doi.org/10.1051/0004-6361/201015082 |
856 | 4 8 | u https://research.chalmers.se/publication/131845 |
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