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The Gaia-ESO Survey: Pre-main-sequence stars in the young open cluster NGC 3293

Authors :
Sergey E. Koposov
S. G. Sousa
A. Hourihane
Alex Lobel
G. G. Sacco
Giovanni Carraro
Emilio J. Alfaro
T. Semaan
L. Morbidelli
A. C. Lanzafame
Jack Lewis
Antonio Frasca
Carmela Lardo
Janet E. Drew
Ettore Flaccomio
V. M. Kalari
Andrew R. Casey
L. Prisinzano
M. T. Costado
Gerard Gilmore
Sofia Randich
J. Eislöffel
Giuseppina Micela
R. D. Jeffries
Antonio Delgado
R. Blomme
J. L. Yun
Antonella Vallenari
Lorenzo Monaco
L. Sampedro
Laura Magrini
Thierry Morel
E. Franciosini
Clare Worley
Gilmore, Gerard [0000-0003-4632-0213]
Koposov, Sergey [0000-0003-2644-135X]
Worley, Clare [0000-0001-9310-2898]
Casey, Andrew [0000-0003-0174-0564]
Apollo - University of Cambridge Repository
European Commission
Leverhulme Trust
European Science Foundation
Ministerio de Economía y Competitividad (España)
Delgado A.J.
Sampedro L.
Alfaro E.J.
Costado M.T.
Yun J.L.
Frasca A.
Lanzafame A.C.
Drew J.E.
Eisloffel 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
Source :
Monthly Notices of the Royal Astronomical Society, Digital.CSIC. Repositorio Institucional del CSIC, instname
Publication Year :
2016
Publisher :
Oxford University Press (OUP), 2016.

Abstract

Delgado, Antonio J. et. al.<br />The 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 H alpha emission, are investigated for them. Marginal presence of H alpha 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.<br />This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell' Istruzione, dell' Universita' e della Ricerca (MIUR) in the form of the grant 'Premiale VLT 2012'. The results presented here benefit from discussions held during the Gaia-ESO workshops and conferences supported by the ESF (European Science Foundation) through the GREAT Research Network Programme. AJD, LS, EJA and MTC acknowledge financial support from the Spanish Ministerio de Economia y Competitividad, through grant AYA2013-40611-P. JLY acknowledges support from FCT (SFRH/BSAB/1423/2014 and UID/FIS/04434/2013). TM acknowledges financial support from Belspo for contract PRODEX GAIA-DPAC.

Details

ISSN :
20134061, 00358711, and 13652966
Database :
OpenAIRE
Journal :
Monthly Notices of the Royal Astronomical Society, Digital.CSIC. Repositorio Institucional del CSIC, instname
Accession number :
edsair.doi.dedup.....7d0e09f32259dd237b340b04b13db7be