Show simple item record

dc.contributor.authorGALLI, P. A. B.
hal.structure.identifierInstituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] [IAG]
dc.contributor.authorTEIXEIRA, R.
hal.structure.identifierM2A 2013
dc.contributor.authorDUCOURANT, C.
dc.contributor.authorBERTOUT, C.
dc.date.issued2013-02
dc.date.conference2012
dc.identifier.issn1743-9213
dc.description.abstractEnTo reliably determine the main physical parameters (masses and ages) of young stars, we must know their distances. While the average distance to nearby star-forming regions (<300 pc) is often known, the distances to individual stars are usually unknown. Individual distances to members of young moving groups can be derived from their radial velocities and proper motions using the convergent-point strategy. We investigate the kinematic properties of the Lupus moving group with the primary objective of deriving individual distances to all group members.
dc.language.isoen
dc.publisherCambridge University Press (CUP)
dc.source.titleAdvancing the Physics of Cosmic Distances, Proceedings of the International Astronomical Union, IAU Symposium, Volume 289, pp. 390-393, 2013
dc.subject.enstars: distances
dc.subject.enstars: kinematics
dc.subject.enstars: pre-main-sequence
dc.subject.enISM: individual (Lupus star-forming region)
dc.title.enKinematic distances of pre-main-sequence stars in the Lupus star-forming region
dc.typeCommunication dans un congrès
dc.identifier.doi10.1017/S1743921312021783
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.journalProceedings of the International Astronomical Union
bordeaux.page390-393
bordeaux.volume289
bordeaux.conference.titleAdvancing the Physics of Cosmic Distances
bordeaux.countryCN
bordeaux.title.proceedingAdvancing the Physics of Cosmic Distances, Proceedings of the International Astronomical Union, IAU Symposium, Volume 289, pp. 390-393, 2013
bordeaux.conference.citybeijing
bordeaux.peerReviewedoui
hal.identifierhal-00832298
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00832298v1
bordeaux.COinSctx_ver=Z39.88-2004&amp;rft_val_fmt=info:ofi/fmt:kev:mtx:journal&amp;rft.btitle=Advancing%20the%20Physics%20of%20Cosmic%20Distances,%20Proceedings%20of%20the%20International%20Astronomical%20Union,%20IAU%20Symposium,%20Volume%20289,%20pp.%20390-393,&amp;rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&amp;rft.date=2013-02&amp;rft.volume=289&amp;rft.spage=390-393&amp;rft.epage=390-393&amp;rft.eissn=1743-9213&amp;rft.issn=1743-9213&amp;rft.au=GALLI,%20P.%20A.%20B.&amp;TEIXEIRA,%20R.&amp;DUCOURANT,%20C.&amp;BERTOUT,%20C.&amp;rft.genre=unknown


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record