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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00010416naa a2201297 4500
001oai:DiVA.org:su-51500
003SwePub
008110110s2010 | |||||||||||000 ||eng|
009oai:research.chalmers.se:ef85a7fc-e8bf-4c51-84d4-3143dca5e896
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-515002 URI
024a https://doi.org/10.1051/0004-6361/2010151032 DOI
024a https://research.chalmers.se/publication/1313702 URI
040 a (SwePub)sud (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Marseille, M. G.u Netherlands Institute for Space Research (SRON),Universita degli Studi di Roma Tor Vergata,University of Rome Tor Vergata4 aut
2451 0a Water abundances in high-mass protostellar envelopes :b Herschel observations with HIFI
264 c 2010-10-01
264 1b EDP Sciences,c 2010
338 a print2 rdacarrier
500 a 71
520 a Aims: We derive the dense core structure and the water abundance in four massive star-forming regions in the hope of understanding the earliest stages of massive star formation. Methods: We present Herschel/HIFI observations of the para-H2O 111-000 and 202-111 and the para-H_218O 111-000 transitions. The envelope contribution to the line profiles is separated from contributions by outflows and foreground clouds. The envelope contribution is modeled with Monte-Carlo radiative transfer codes for dust and molecular lines (MC3D and RATRAN), and the water abundance and the turbulent velocity width as free parameters. Results: While the outflows are mostly seen in emission in high-J lines, envelopes are seen in absorption in ground-state lines, which are almost saturated. The derived water abundances range from 5×10-10 to 4×10-8 in the outer envelopes. We detect cold clouds surrounding the protostar envelope, thanks to the very high quality of the Herschel/HIFI data and the unique ability of water to probe them. Several foreground clouds are also detected along the line of sight. Conclusions: The low H2O abundances in massive dense cores are in accordance with the expectation that high densities and low temperatures lead to freeze-out of water on dust grains. The spread in abundance values is not clearly linked to physical properties of the sources. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation of NASA.Appendix (pages 6 to 7) is only available in electronic form at http://www.aanda.org
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 dust
653 a extinction
653 a ISM: molecules
653 a ISM: abundances
653 a Astronomy and astrophysics
653 a Astronomi och astrofysik
653 a Astronomy
653 a astronomi
700a van der Tak, F. F. S.u Rijksuniversiteit Groningen,University of Groningen,Netherlands Institute for Space Research (SRON)4 aut
700a Herpin, F.u Institut National des Sciences de l'Univers,Laboratoire d'Astrophysique de Bordeaux4 aut
700a Wyrowski, F.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG),Netherlands Institute for Space Research (SRON)4 aut
700a Chavarría, L.u Laboratoire d'Astrophysique de Bordeaux,Institut National des Sciences de l'Univers4 aut
700a Pietropaoli, B.u Laboratoire d'Astrophysique de Bordeaux,Institut National des Sciences de l'Univers4 aut
700a Baudry, A.u Laboratoire d'Astrophysique de Bordeaux,Institut National des Sciences de l'Univers4 aut
700a Bontemps, S.u Laboratoire d'Astrophysique de Bordeaux,Institut National des Sciences de l'Univers4 aut
700a Cernicharo, J.u Centro de Astrobiologia (CAB)4 aut
700a Jacq, T.u Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory4 aut
700a Frieswijk, W.u Eidgenössische Technische Hochschule Zürich (ETH),Swiss Federal Institute of Technology in Zürich (ETH)4 aut
700a Shipman, R.u Netherlands Institute for Space Research (SRON)4 aut
700a van Dishoeck, E. F.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG),Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Bachiller, R.u Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)4 aut
700a Benedettini, M.u Universita degli Studi di Roma Tor Vergata,University of Rome Tor Vergata4 aut
700a Benz, A. O.u Eidgenössische Technische Hochschule Zürich (ETH),Swiss Federal Institute of Technology in Zürich (ETH)4 aut
700a Bergin, E.u University of Michigan4 aut
700a Bjerkeli, Per,d 1977u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)gu97pebj
700a Blake, G. A.u California Institute of Technology (Caltech)4 aut
700a Braine, J.u Laboratoire d'Astrophysique de Bordeaux,Institut National des Sciences de l'Univers,Netherlands Institute for Space Research (SRON)4 aut
700a Bruderer, S.u Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory,University of Leeds4 aut
700a Caselli, P.u California Institute of Technology (Caltech),Institut National des Sciences de l'Univers,Laboratoire d'Astrophysique de Bordeaux4 aut
700a Caux, E.u Institut National des Sciences de l'Univers,Université de Toulouse,University of Toulouse4 aut
700a Codella, C.u Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory,Radboud Universiteit,Radboud University,Anton Pannekoek Institute for Astronomy,Western University,University of Waterloo,Netherlands Institute for Space Research (SRON)4 aut
700a Daniel, F.u Centro de Astrobiologia (CAB)4 aut
700a Dieleman, P.u Netherlands Institute for Space Research (SRON)4 aut
700a di Giorgio, A. M.u Eidgenössische Technische Hochschule Zürich (ETH),Swiss Federal Institute of Technology in Zürich (ETH)4 aut
700a Dominik, C.4 aut
700a Doty, S. D.u Denison University4 aut
700a Encrenaz, P.u LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France4 aut
700a Fich, M.u University of Waterloo4 aut
700a Fuente, A.u Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)4 aut
700a Gaier, T.4 aut
700a Giannini, T.u Osservatorio Astronomico di Roma4 aut
700a Goicoechea, J. R.u Centro de Astrobiologia (CAB)4 aut
700a de Graauw, Th.u Netherlands Institute for Space Research (SRON)4 aut
700a Helmich, F.u Netherlands Institute for Space Research (SRON)4 aut
700a Herczeg, G. J.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Hogerheijde, M. R.u Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Jackson, B.4 aut
700a Javadi, H.4 aut
700a Jellema, W.u Netherlands Institute for Space Research (SRON)4 aut
700a Johnstone, D.u National Research Council Canada,University of Victoria4 aut
700a Jørgensen, J. K.u Köpenhamns universitet,University of Copenhagen4 aut
700a Kester, D.u Netherlands Institute for Space Research (SRON)4 aut
700a Kristensen, L. E.u Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Larsson, Bengtu Stockholms universitet,Institutionen för astronomi,Stockholm University4 aut0 (Swepub:su)bem
700a Laauwen, W.u Netherlands Institute for Space Research (SRON)4 aut
700a Lis, D.u California Institute of Technology (Caltech)4 aut
700a Liseau, René,d 1949u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)liseau
700a Luinge, W.u Netherlands Institute for Space Research (SRON)4 aut
700a McCoey, C.4 aut
700a Megej, A.4 aut
700a Melnick, G.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Neufeld, D.u Johns Hopkins University4 aut
700a Nisini, B.u Osservatorio Astronomico di Roma4 aut
700a Olberg, Michael,d 1956u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)olberg
700a Parise, B.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Pearson, J. C.4 aut
700a Plume, R.u University of Calgary,Netherlands Institute for Space Research (SRON)4 aut
700a Risacher, C.4 aut
700a Roelfsema, P.4 aut
700a Santiago-García, J.u Institut de Radioastronomie Millimétrique (IRAM)4 aut
700a Saraceno, P.u Universita degli Studi di Roma Tor Vergata,University of Rome Tor Vergata4 aut
700a Siegel, P.4 aut
700a Stutzki, J.u Universität zu Köln,University of Cologne4 aut
700a Tafalla, M.u Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)4 aut
700a van Kempen, T. A.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Visser, R.u Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Wampfler, S. F.4 aut
700a Yıldız, U. A.u Universiteit Leiden (UL),Leiden University (UL)4 aut
710a Netherlands Institute for Space Research (SRON)b Universita degli Studi di Roma Tor Vergata4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 521, s. L32-q 521<L32-x 0004-6361x 1432-0746
856u https://www.aanda.org/articles/aa/pdf/2010/13/aa15103-10.pdf
856u http://publications.lib.chalmers.se/records/fulltext/local_131370.pdfx primaryx freey FULLTEXT
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-51500
8564 8u https://doi.org/10.1051/0004-6361/201015103
8564 8u https://research.chalmers.se/publication/131370

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