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dc.contributor.authorGalvez-Ortiz, M. C.
dc.contributor.authorClarke, J. R. A.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorFolkes, S. L.
dc.contributor.authorJenkins, J. S.
dc.contributor.authorPerez, A. E. Garcia
dc.contributor.authorBurningham, B.
dc.contributor.authorDay-Jones, A. C.
dc.contributor.authorJones, H.R.A.
dc.contributor.editorDuForesto, V C
dc.contributor.editorGelino, D M
dc.contributor.editorRibas, I
dc.date.accessioned2012-01-18T10:01:12Z
dc.date.available2012-01-18T10:01:12Z
dc.date.issued2010
dc.identifier.citationGalvez-Ortiz , M C , Clarke , J R A , Pinfield , D J , Folkes , S L , Jenkins , J S , Perez , A E G , Burningham , B , Day-Jones , A C & Jones , H R A 2010 , Low-mass Objects in Moving Groups . in V C DuForesto , D M Gelino & I Ribas (eds) , Pathways Towards Habitable Planets . ASP Conf Series , vol. 430 , Astronomical Society of the Pacific , pp. 434-436 , Barcelona Conference on Pathways Towards Habitable Planets , Barcelona , 14/09/09 .
dc.identifier.citationconference
dc.identifier.isbn978-1-58381-740-7
dc.identifier.isbn978-1-58381-741-4
dc.identifier.otherPURE: 527431
dc.identifier.otherPURE UUID: 82128be1-d73f-4a44-9af0-f1bc2c9e0497
dc.identifier.otherWOS: 000287836800072
dc.identifier.otherORCID: /0000-0003-4600-5627/work/64327361
dc.identifier.urihttp://hdl.handle.net/2299/7680
dc.description.abstractWe present here the kinematic study of part of a 132 target sample of low-mass objects, previously selected by photometric and astrometric criteria as possible members to five young moving groups (MGs): Local Association (Pleiades moving group, 20 - 150 Myr), Ursa Mayor group (Sirius supercluster, 300 Myr), Hyades supercluster (600 Myr), IC 2391 supercluster (35 Myr) and Castor moving group (200 Myr). We calculated their kinematic galactic components (U,V,W) and apply simple kinematic criteria of membership. The confirmed members will provide a new and substantial population of age and metallicity benchmark ultra cool dwarfs (UCDs). This will give a valuable set to test atmosphere and evolutionary models of ages below 1 Gyr and suitable targets for use in adaptive optic (AO) imaging to search for sub-stellar companions/exoplanets.en
dc.format.extent3
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofPathways Towards Habitable Planets
dc.relation.ispartofseriesASP Conf Series
dc.subjectmembers
dc.subjectstars : activity
dc.titleLow-mass Objects in Moving Groupsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
rioxxterms.versionVoR
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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