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hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorBOSELLI, A.
hal.structure.identifierMax-Planck-Institut für Extraterrestrische Physik [MPE]
dc.contributor.authorFOSSATI, M.
hal.structure.identifierDepartment of Civil Engineering
dc.contributor.authorLONGOBARDI, A.
hal.structure.identifierUniversità degli Studi di Milano-Bicocca = University of Milano-Bicocca [UNIMIB]
dc.contributor.authorCONSOLANDI, G.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorAMRAM, P.
hal.structure.identifierMinistry of Agriculture of the People's Republic of China [MOA]
dc.contributor.authorSUN, M.
hal.structure.identifierEuropean Southern Observatory [ESO]
dc.contributor.authorANDREANI, P.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorBOQUIEN, M.
hal.structure.identifierFORMATION STELLAIRE 2019
dc.contributor.authorBRAINE, J.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
hal.structure.identifierCollège de France - Chaire Galaxies et cosmologie
dc.contributor.authorCOMBES, F.
hal.structure.identifierNRC Herzberg Astronomy and Astrophysics
dc.contributor.authorCOTE, P.
hal.structure.identifierCanada-France-Hawaii Telescope Corporation [CFHT]
dc.contributor.authorCUILLANDRE, J. C.
hal.structure.identifierDépartement d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA]
dc.contributor.authorDUC, P.A.
dc.contributor.authorEMSELLEM, E.
hal.structure.identifierNRC Herzberg Institute of Astrophysics
dc.contributor.authorFERRARESE, L.
dc.contributor.authorGAVAZZI, G.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA (UMR_8112)]
dc.contributor.authorGWYN, S.
hal.structure.identifierUniversity of Vienna [Vienna]
dc.contributor.authorHENSLER, G.
dc.contributor.authorPENG, E. W.
hal.structure.identifierLaboratorio de Astrofísica Teórica e Observacional
dc.contributor.authorPLANA, H.
dc.contributor.authorROEDIGER, J.
dc.contributor.authorSANCHEZ-JANSSEN, R.
dc.contributor.authorSARZI, M.
dc.contributor.authorSERRA, P.
dc.contributor.authorTRINCHIERI, G.
dc.date.issued2019-03
dc.identifier.issn0004-6361
dc.description.abstractEnWe observed the giant elliptical galaxy M 87 during 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 Canada French Hawaii Telescope (CFHT). The deep narrow-band image confirmed the presence of a filament of ionised gas extending up to ≃3 kpc in the north-western direction and ≃8 kpc to the southeast, with a couple of plumes of ionised gas, the weakest of which, at ≃18 kpc from the nucleus, was previously unknown. The analysis of deep optical images taken from the NGVS survey confirms that this gas filament is associated with dust seen in absorption which is now detected up to ≃2.4 kpc from the nucleus. We also analysed the physical and kinematical properties of the ionised gas filament using deep IFU MUSE data covering the central 4.8 × 4.8 kpc2 of the galaxy. The spectroscopic data confirm a perturbed kinematics of the ionised gas, with differences in velocity of ≃700–800 km s−1 on scales of ≲1 kpc. The analysis of 2D diagnostic diagrams and the observed relationship between the shock-sensitive [OI]/Hα line ratio and the velocity dispersion of the gas suggest that the gas is shock-ionised.
dc.language.isoen
dc.publisherEDP Sciences
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.subject.engalaxies: clusters: general
dc.subject.engalaxies: clusters: individual: Virgo
dc.subject.engalaxies: evolution
dc.subject.engalaxies: interactions
dc.subject.engalaxies: ISM
dc.subject.engalaxies: individual: M 87
dc.title.enA Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)
dc.title.enV. Properties of the ionised gas filament of M 87
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201834492
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1810.09804
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageA52
bordeaux.volume623
bordeaux.peerReviewedoui
hal.identifierhal-01903254
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01903254v1
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