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The nearest young moving groups

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dc.contributor.authorLópez Santiago, Javier
dc.contributor.authorMontes Gutiérrez, David
dc.contributor.authorCrespo Chacón, I.
dc.contributor.authorFernández Figueroa, María José
dc.date.accessioned2023-06-20T10:58:03Z
dc.date.available2023-06-20T10:58:03Z
dc.date.issued2006-06-01
dc.description© 2006. The American Astronomical Society. All rights reserved. This work was supported by the Universidad Complutense de Madrid and the Spanish Ministerio de Educación y Ciencia (MEC), Programa Nacional de Astronomía y Astrofísica under grants AYA 2004-03749 and AYA 2005-02750. I. C. C. acknowledges support from MEC under AP2001-0475. We would like to thank the referee for useful comments that have helped improve the manuscript.
dc.description.abstractThe latest results in the research of forming planetary systems have led several authors to compile a sample of candidates for searching for planets in the vicinity of the Sun. Young stellar associations are indeed excellent laboratories for this study, but some of them are not close enough to allow the detection of planets through adaptive optics techniques. However, the existence of very close young moving groups can solve this problem. Here we have compiled the members of the nearest young moving groups, as well as a list of new candidates from our catalog of late-type stars that are possible members of young stellar kinematic groups, studying their membership through spectroscopic and photometric criteria.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUniversidad Complutense de Madrid (UCM)
dc.description.sponsorshipMinisterio de Educación y Ciencia (MEC), España
dc.description.sponsorshipPrograma Nacional de Astronomía y Astrofísica (MCYT)
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/31477
dc.identifier.doi10.1086/503183
dc.identifier.issn0004-637X
dc.identifier.officialurlhttp://dx.doi.org/10.1086/503183
dc.identifier.relatedurlhttp://iopscience.iop.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/51527
dc.issue.number2
dc.journal.titleAstrophysical journal
dc.language.isoeng
dc.page.final1165
dc.page.initial1160
dc.publisherAmerican Astronomical Society
dc.relation.projectIDAYA 2004-03749
dc.relation.projectIDAYA 2005-02750
dc.relation.projectIDAP2001-0475
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordStellar velocity distribution
dc.subject.keywordLocal association
dc.subject.keywordSolar neighborhood
dc.subject.keywordAB-doradus
dc.subject.keywordKinematic groups
dc.subject.keywordMass stars
dc.subject.keywordNearby
dc.subject.keywordAge
dc.subject.keywordPleiades
dc.subject.keywordSystem
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleThe nearest young moving groups
dc.typejournal article
dc.volume.number643
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