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dc.contributor.authorGALLI, P. A. B.
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorBERTOUT, C.
hal.structure.identifierInstituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] [IAG]
dc.contributor.authorTEIXEIRA, R.
hal.structure.identifierM2A 2014
dc.contributor.authorDUCOURANT, C.
dc.date.issued2014-10
dc.date.conference2013
dc.description.abstractEnIn this paper, we study the southern star-forming region located in Lupus that constitutes one of the richest associations of T Tauri stars. Based on the convergent point (CP) method combined with a k-NN analysis we identify 109 pre-main sequence stars in this region that define the Lupus association of comoving stars, and derive individual distances for all group members.
dc.language.isoen
dc.title.enA kinematic study of the Lupus star-forming region
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.page28 - 28
bordeaux.volume44
bordeaux.conference.titleXIV Latin American Regional IAU Meeting (Eds. A. Mateus, J. Gregorio-Hetem & R. Cid Fernandes) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 44, pp. 28-28 (2014) held Florianópolis, Brasil, November 24 - 30, 2013
bordeaux.countryBR
bordeaux.conference.cityFlorianópolis
bordeaux.peerReviewedoui
hal.identifierhal-01092364
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01092364v1
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