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

Autor: 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
Přispěvatelé: 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
Rok vydání: 2016
Předmět:
Zdroj: Monthly Notices of the Royal Astronomical Society
Digital.CSIC. Repositorio Institucional del CSIC
instname
ISSN: 2013-4061
0035-8711
1365-2966
Popis: Delgado, Antonio J. et. al.
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.
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.
Databáze: OpenAIRE
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