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T Tauri Disk Lifetime in the Lupus Association

hal.structure.identifierInstituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] [IAG]
dc.contributor.authorGALLI, P. A. B.
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorBERTOUT, C.
dc.contributor.authorTEIXEIRA, R.
hal.structure.identifierM2A 2015
dc.contributor.authorDUCOURANT, C.
dc.date.issued2015-11
dc.date.conference2016-05-11
dc.description.abstractEnIn a recent study, we derived individual distances for a sample of pre-main sequence stars that define the comoving association of young stars in the Lupus star-forming region. Here, we use these new distances to investigate the mass and age distributions of Lupus T Tauri stars and derive the average disk lifetime in the Lupus association based on an empirical disk model.
dc.language.isoen
dc.title.enT Tauri Disk Lifetime in the Lupus Association
dc.typeCommunication dans un congrès
dc.identifier.doi10.1017/S1743921315006262
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.volume10
bordeaux.issueS314
bordeaux.conference.titleYoung Stars & Planets Near the Sun, Proceedings of the International Astronomical Union, IAU Symposium, Volume 314, pp. 191-192- held 11 - 15 May 2015 / U.S.A, Atlanta, GA (Cambridge University Press), J.H. Kastner, B. Stelzer, S.A. Metchev, eds
bordeaux.countryUS
bordeaux.conference.cityAtlanta
bordeaux.peerReviewedoui
hal.identifierhal-01266214
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01266214v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2015-11&rft.volume=10&rft.issue=S314&rft.au=GALLI,%20P.%20A.%20B.&BERTOUT,%20C.&TEIXEIRA,%20R.&DUCOURANT,%20C.&rft.genre=unknown


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