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dc.contributor.authorDelgado, A. J.
dc.contributor.authorSampedro, L.
dc.contributor.authorAlfaro, E. J.
dc.contributor.authorCostado, M. T.
dc.contributor.authorYun, J. L.
dc.contributor.authorFrasca, A.
dc.contributor.authorLanzafame, A. C.
dc.contributor.authorDrew, J. E.
dc.contributor.authorEislöffel, J.
dc.contributor.authorBlomme, R.
dc.contributor.authorMorel, T.
dc.contributor.authorLobel, A.
dc.contributor.authorSemaan, T.
dc.contributor.authorRandich, S.
dc.contributor.authorJeffries, R. D.
dc.contributor.authorMicela, G.
dc.contributor.authorVallenari, A.
dc.contributor.authorKalari, V.
dc.contributor.authorGilmore, G.
dc.contributor.authorFlaccomio, E.
dc.contributor.authorCarraro, G.
dc.contributor.authorLardo, C.
dc.contributor.authorMonaco, L.
dc.contributor.authorPrisinzano, L.
dc.contributor.authorSousa, S. G.
dc.contributor.authorMorbidelli, L.
dc.contributor.authorLewis, J.
dc.contributor.authorKoposov, S.
dc.contributor.authorHourihane, A.
dc.contributor.authorWorley, C.
dc.contributor.authorCasey, A.
dc.contributor.authorFranciosini, E.
dc.contributor.authorSacco, G.
dc.contributor.authorMagrini, L.
dc.date.accessioned2017-05-04T17:03:29Z
dc.date.available2017-05-04T17:03:29Z
dc.date.issued2016-08-11
dc.identifier.citationDelgado , A J , Sampedro , L , Alfaro , E J , Costado , M T , Yun , J L , Frasca , A , Lanzafame , A C , Drew , J E , Eislöffel , J , Blomme , R , Morel , T , Lobel , A , Semaan , T , Randich , S , Jeffries , R D , Micela , G , Vallenari , A , Kalari , V , Gilmore , G , Flaccomio , E , Carraro , G , Lardo , C , Monaco , L , Prisinzano , L , Sousa , S G , Morbidelli , L , Lewis , J , Koposov , S , Hourihane , A , Worley , C , Casey , A , Franciosini , E , Sacco , G & Magrini , L 2016 , ' The Gaia-ESO Survey: pre-main-sequence stars in the young open cluster NGC 3293 ' , Monthly Notices of the Royal Astronomical Society , vol. 460 , no. 3 , pp. 3305-3315 . https://doi.org/10.1093/mnras/stw1217
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 10537346
dc.identifier.otherPURE UUID: ac87e106-7380-467b-a89e-d3d61cfc569c
dc.identifier.otherScopus: 84983247319
dc.identifier.urihttp://hdl.handle.net/2299/18158
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. The version of record [A. J. Delgado, et al, 'The Gaia-ESO Survey: pre-main-sequence stars in the young open cluster NGC 3293', Monthly Notices of the Royal Astronomical Society, Vol. 460(3): 3305-3315, first published online 20 May 2016] is available online at doi: https://doi.org/10.1093/mnras/stw1217. © 2016 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
dc.description.abstractThe young open cluster NGC3293 is included in the observing program of the Gaia-ESO survey (GES). The radial velocity values provided have been used to assign cluster membership probabilities by means of a single-variable parametric analysis. These membership probabilities are compared to the results of the photometric membership assignment of NGC3293, based on UBVRI photometry. The agreement of the photometric and kinematic member samples amounts to 65 per cent, and could increase to 70 per cent as suggested by the analysis of the differences between both samples. A number of photometric PMS candidate members of spectral type F are found, which are confirmed by the results from VPHAS photometry and SED fitting for the stars in common with VPHAS and GES data sets. Excesses at mid- and near-infrared wavelengths, and signs of Hα emission, are investigated for them. Marginal presence of Hα emission or infilling is detected for the candidate members. Several of them exhibit moderate signs of U excess and weak excesses at mid-IR wavelengths. We suggest that these features originate from accretion discs in their last stages of evolution.en
dc.format.extent11
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsOpen
dc.subjectOpen clusters and associations: general
dc.subjectOpen clusters and associations: individual: NGC 3293
dc.subjectStars: pre-main-sequence
dc.subjectAstronomy and Astrophysics
dc.titleThe Gaia-ESO Survey: pre-main-sequence stars in the young open cluster NGC 3293en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionUniversity of Hertfordshire
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=84983247319&partnerID=8YFLogxK
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2016-08-11
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stw1217
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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