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hal.structure.identifierSRON Netherlands Institute for Space Research [SRON]
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorVAN DER TAK, Floris
hal.structure.identifierFORMATION STELLAIRE 2011
dc.contributor.authorHERPIN, Fabrice
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorWYROWSKI, Friedrich
dc.contributor.authorFOR THE HIGH-MASS WISH TEAM
dc.date.issued2011
dc.date.conference2010
dc.description.abstractEnThis paper reviews the first results of observations of H2O line emission with Herschel-HIFI towards high-mass star-forming regions, obtained within the WISH guaranteed time program. The data reveal three kinds of gas-phase H2O: 'cloud water' in cold tenuous foreground clouds, 'envelope water' in dense protostellar envelopes, and 'outflow water' in protostellar outflows. The low H2O abundance (1e-10 -- 1e-9) in foreground clouds and protostellar envelopes is due to rapid photodissociation and freeze-out on dust grains, respectively. The outflows show higher H2O abundances (1e-7 -- 1e-6) due to grain mantle evaporation and (probably) neutral-neutral reactions.
dc.language.isoen
dc.source.titleEAS Publications Series, Volume 52, 2011, pp.201-204
dc.subject.enAstrophysics
dc.subject.enGalaxy Astrophysics
dc.title.enHerschel-HIFI observations of H2O in high-mass star-forming regions: first results
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
bordeaux.page201-204
bordeaux.volume52
bordeaux.conference.titleConditions and Impact of Star Formation
bordeaux.countryCH
bordeaux.title.proceedingEAS Publications Series, Volume 52, 2011, pp.201-204
bordeaux.conference.cityZermatt
bordeaux.peerReviewedoui
hal.identifierhal-00553002
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00553002v1
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