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hal.structure.identifierSwedish Institute of Space Physics [Kiruna] [IRF]
dc.contributor.authorHOLMSTRÖM, M.
hal.structure.identifierSwedish Institute of Space Physics [Kiruna] [IRF]
dc.contributor.authorEKENBÄCK, A.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorSELSIS, Franck
hal.structure.identifierINAF - Osservatorio Astronomico di Palermo [OAPa]
dc.contributor.authorPENZ, T.
dc.contributor.authorLAMMER, H.
hal.structure.identifierPhysikalisches Institut [Bern]
dc.contributor.authorWURZ, P.
dc.date.created2008
dc.date.issued2008
dc.identifier.issn0028-0836
dc.description.abstractEnLecavelier des Etangs et al. 1 object to the conclusion by Holmström et al. 2 that radiation pressure alone cannot explain the Lyman- absorption observed3 during transits of HD 209458b. We agree that hydrogen atoms can be accelerated to large velocities by radiation pressure. However, with our model we cannot reproduce the observed spectrum, as shown in the Supplementary Information and Fig. 3 of ref. 2.
dc.language.isoen
dc.publisherNature Publishing Group
dc.title.enThe origin of hydrogen around HD 209458b
dc.typeArticle de revue
dc.identifier.doi10.1038/nature07402
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv0902.3994
bordeaux.journalNature
bordeaux.pageE1-E2
bordeaux.issue456
bordeaux.peerReviewedoui
hal.identifierhal-00338388
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00338388v1
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