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dc.rights.licenseopenen_US
dc.contributor.authorBOSELLI, A.
dc.contributor.authorFOSSATI, M.
dc.contributor.authorCUILLANDRE, J. C.
dc.contributor.authorBOISSIER, S.
dc.contributor.authorBOQUIEN, M.
dc.contributor.authorBUAT, V.
dc.contributor.authorBURGARELLA, D.
dc.contributor.authorCONSOLANDI, G.
dc.contributor.authorCORTESE, L.
dc.contributor.authorCOTE, P.
hal.structure.identifierBordeaux population health [BPH]
dc.contributor.authorCOTE, Sylvana
dc.contributor.authorDURRELL, P.
dc.contributor.authorFERRARESE, L.
dc.contributor.authorFUMAGALLI, M.
dc.contributor.authorGAVAZZI, G.
dc.contributor.authorGWYN, S.
dc.contributor.authorHENSLER, G.
dc.contributor.authorKORIBALSKI, B.
dc.contributor.authorROEDIGER, J.
dc.contributor.authorROEHLLY, Y.
dc.contributor.authorRUSSEIL, D.
dc.contributor.authorSUN, M.
dc.contributor.authorTOLOBA, E.
dc.contributor.authorVOLLMER, B.
dc.contributor.authorZAVAGNO, A.
dc.date.accessioned2021-04-23T09:06:33Z
dc.date.available2021-04-23T09:06:33Z
dc.date.issued2018
dc.identifier.issn0004-6361en_US
dc.identifier.urihttps://oskar-bordeaux.fr/handle/20.500.12278/27067
dc.description.abstractEnDuring pilot observations of the Virgo Environmental Survey Tracing Galaxy Evolution (VESTIGE), a blind narrow-band Hα + [NII] imaging survey of the Virgo cluster carried out with MegaCam at the CFHT, we have observed the spiral galaxy NGC 4254 (M99). Deep Hα + [NII] narrow-band and GALEX UV images reveal the presence of 60 compact (70–500 pc radius) star-forming regions up to ≃20 kpc outside the optical disc of the galaxy. These regions are located along a tail of HI gas stripped from the disc of the galaxy after a rapid gravitational encounter with another Virgo cluster member that simulations indicate occurred 280–750 Myr ago. We have combined the VESTIGE data with multifrequency data from the UV to the far-infrared to characterise the stellar populations of these regions and study the star formation process in an extreme environment such as the tails of stripped gas embedded in the hot intracluster medium. The colour, spectral energy distribution (SED), and linear size consistently indicate that these regions are coeval and have been formed after a single burst of star formation that occurred ≲100 Myr ago. These regions might become free floating objects within the cluster potential well, and be the local analogues of compact sources produced after the interaction of gas-rich systems that occurred during the early formation of clusters.
dc.language.isoENen_US
dc.subject.engalaxies: individual: NGC 4254
dc.subject.engalaxies: clusters: general
dc.subject.engalaxies: clusters: individual: Virgo
dc.subject.engalaxies: evolution
dc.subject.engalaxies: interactions
dc.subject.engalaxies: ISM
dc.title.enA Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)
dc.title.enIII. Star formation in the stripped gas of NGC 4254
dc.typeArticle de revueen_US
dc.identifier.doi10.1051/0004-6361/201732410en_US
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]en_US
bordeaux.journalAstronomy and Astrophysics - A&Aen_US
bordeaux.pageA114en_US
bordeaux.volume615en_US
bordeaux.hal.laboratoriesBordeaux Population Health Research Center (BPH) - UMR 1219en_US
bordeaux.institutionUniversité de Bordeauxen_US
bordeaux.institutionINSERMen_US
bordeaux.teamHEALTHY_BPHen_US
bordeaux.peerReviewedouien_US
bordeaux.inpressnonen_US
bordeaux.import.sourcehal
hal.identifierhal-03000032
hal.version1
hal.exportfalse
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