Kinematic distances of pre-main-sequence stars in the Lupus star-forming region
dc.contributor.author | GALLI, P. A. B. | |
hal.structure.identifier | Instituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] [IAG] | |
dc.contributor.author | TEIXEIRA, R. | |
hal.structure.identifier | M2A 2013 | |
dc.contributor.author | DUCOURANT, C. | |
dc.contributor.author | BERTOUT, C. | |
dc.date.issued | 2013-02 | |
dc.date.conference | 2012 | |
dc.identifier.issn | 1743-9213 | |
dc.description.abstractEn | To 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.iso | en | |
dc.publisher | Cambridge University Press (CUP) | |
dc.source.title | Advancing the Physics of Cosmic Distances, Proceedings of the International Astronomical Union, IAU Symposium, Volume 289, pp. 390-393, 2013 | |
dc.subject.en | stars: distances | |
dc.subject.en | stars: kinematics | |
dc.subject.en | stars: pre-main-sequence | |
dc.subject.en | ISM: individual (Lupus star-forming region) | |
dc.title.en | Kinematic distances of pre-main-sequence stars in the Lupus star-forming region | |
dc.type | Communication dans un congrès | |
dc.identifier.doi | 10.1017/S1743921312021783 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM] | |
bordeaux.journal | Proceedings of the International Astronomical Union | |
bordeaux.page | 390-393 | |
bordeaux.volume | 289 | |
bordeaux.conference.title | Advancing the Physics of Cosmic Distances | |
bordeaux.country | CN | |
bordeaux.title.proceeding | Advancing the Physics of Cosmic Distances, Proceedings of the International Astronomical Union, IAU Symposium, Volume 289, pp. 390-393, 2013 | |
bordeaux.conference.city | beijing | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00832298 | |
hal.version | 1 | |
hal.invited | non | |
hal.proceedings | oui | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00832298v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=Advancing%20the%20Physics%20of%20Cosmic%20Distances,%20Proceedings%20of%20the%20International%20Astronomical%20Union,%20IAU%20Symposium,%20Volume%20289,%20pp.%20390-393,&rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&rft.date=2013-02&rft.volume=289&rft.spage=390-393&rft.epage=390-393&rft.eissn=1743-9213&rft.issn=1743-9213&rft.au=GALLI,%20P.%20A.%20B.&TEIXEIRA,%20R.&DUCOURANT,%20C.&BERTOUT,%20C.&rft.genre=unknown |
Files in this item
Files | Size | Format | View |
---|---|---|---|
There are no files associated with this item. |