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Unravelling the luminosity distribution of IC 4665

hal.structure.identifierM2A 2018
dc.contributor.authorMIRET-ROIG, N.
hal.structure.identifierM2A 2018
dc.contributor.authorBOUY, H.
hal.structure.identifierM2A 2018
dc.contributor.authorOLIVARES, J.
dc.date.issued2018
dc.date.conference2018-07-03
dc.description.abstractEnThe study of star formation is extremely challenging due to the lack of complete and low-contaminated samples of young, nearby, clusters and star forming regions. We aim at providing a membership analysis with a high completeness and low contamination of the young, nearby, open cluster IC4665. We apply modern Bayesian statistical tools to the recent Gaia DR2 catalogue to identify high probability members. We find a list of 543 members of IC4665 with membership probabilities >87%, 251 of which are new members. We compute the magnitude distribution of these sample which peaks at G˜10, equivalent to ˜0.25 M_⊙.
dc.language.isoen
dc.subject.enStars: luminosity function
dc.subject.enGalaxy: open clusters and associations: individual: IC4665
dc.title.enUnravelling the luminosity distribution of IC 4665
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.countryFR
bordeaux.conference.cityBORDEAUX
bordeaux.peerReviewedoui
hal.identifierhal-01982141
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01982141v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2018&rft.au=MIRET-ROIG,%20N.&BOUY,%20H.&OLIVARES,%20J.&rft.genre=unknown


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