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The VLT-FLAMES Tarantula Survey

dc.contributor.authorEvans, C. J.
dc.contributor.authorLennon, D.
dc.contributor.authorLanger, N.
dc.contributor.authorAlmeida, L.
dc.contributor.authorBartlett, E.
dc.contributor.authorBastian, N.
dc.contributor.authorBestenlehner, J. M.
dc.contributor.authorBritavskiy, N.
dc.contributor.authorCastro, N.
dc.contributor.authorClark, S.
dc.contributor.authorCrowther, P. A.
dc.contributor.authorDe Koter, A.
dc.contributor.authorDe Mink, S.
dc.contributor.authorDufton, P. L.
dc.contributor.authorFossati, L.
dc.contributor.authorGarcía, M.
dc.contributor.authorGieles, M.
dc.contributor.authorGräfener, G.
dc.contributor.authorGrin, N.
dc.contributor.authorHénault Brunet, V.
dc.contributor.authorHerrero, A.
dc.contributor.authorHowarth, I.
dc.contributor.authorIzzard, R.
dc.contributor.authorKalari, V.
dc.contributor.authorMaíz Apellániz, J.
dc.contributor.authorMarkova, N.
dc.contributor.authorNajarro, F.
dc.contributor.authorPatrick, Lee R.
dc.contributor.authorPuls, J.
dc.contributor.authorRamírez Agudelo, O.
dc.contributor.authorRenzo, M.
dc.contributor.authorSabín Sanjulián, C.
dc.contributor.authorSana, H.
dc.contributor.authorSchneider, F.
dc.contributor.authorSchootemeijer, A.
dc.contributor.authorSimón Díaz, S.
dc.contributor.authorSmartt, S.
dc.contributor.authorTaylor, W.
dc.contributor.authorTramper, F.
dc.contributor.authorVan Loon, J.
dc.contributor.authorVillaseñor, J.
dc.contributor.authorVink, J. S.
dc.contributor.authorWalborn, N.
dc.date.accessioned2021-04-12T10:17:54Z
dc.date.available2021-04-12T10:17:54Z
dc.date.issued2020-09-01
dc.description6 pageses
dc.description.abstractThe VLT-FLAMES Tarantula Survey (VFTS) was an ESO Large Programme that has provided a rich, legacy dataset for studies of both resolved and integrated populations of massive stars. Initiated in 2008 (ESO Period 82), we used the Fibre Large Array Multi Element Spectrograph (FLAMES) to observe more than 800 massive stars in the dramatic 30 Doradus star-forming region in the Large Magellanic Cloud. At the start of the survey the importance of multiplicity among high-mass stars was becoming evident, so a key feature was multi-epoch spectroscopy to detect radial-velocity shifts arising from binary motion. Here we summarise some of the highlights from the survey and look ahead to the future of the field.es
dc.description.peerreviewedPeer reviewes
dc.identifier.citationThe Messenger 181: 22-27(2020)es
dc.identifier.doi10.18727/0722-6691/5207
dc.identifier.e-issn0722-6691
dc.identifier.issn1209-7233
dc.identifier.otherhttp://doi.eso.org/10.18727/0722-6691/5207
dc.identifier.urihttp://hdl.handle.net/20.500.12666/244
dc.language.isoenges
dc.publisherAstronomical Sciencees
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationales
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.rights.licenseCopyright European Southern Observatory
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleThe VLT-FLAMES Tarantula Surveyes
dc.typeinfo:eu-repo/semantics/articlees
dc.type.coarhttp://purl.org/coar/resource_type/c_6501
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion
dspace.entity.typePublication

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