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Benchmark low-mass objects in Moving Groups

dc.contributor.authorGalvez-Ortiz, M. C.
dc.contributor.authorKuznetsov, M.
dc.contributor.authorClarke, J. R. A.
dc.contributor.authorPavlenko, Ya. V.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorJenkins, J. S.
dc.contributor.authorBarnes, J.
dc.contributor.authorBurningham, B.
dc.contributor.authorDay-Jones, A. C.
dc.contributor.authorMartin, E. L.
dc.contributor.authorPerez, A. E. Garcia
dc.contributor.authorPokorny, R.S.
dc.contributor.editorSaglia, R.
dc.date.accessioned2014-07-14T14:30:18Z
dc.date.available2014-07-14T14:30:18Z
dc.date.issued2013
dc.identifier.citationGalvez-Ortiz , M C , Kuznetsov , M , Clarke , J R A , Pavlenko , Y V , Pinfield , D J , Jones , H R A , Jenkins , J S , Barnes , J , Burningham , B , Day-Jones , A C , Martin , E L , Perez , A E G & Pokorny , R S 2013 , Benchmark low-mass objects in Moving Groups . in R Saglia (ed.) , Hot Planets and Cool Stars . , 05007 , EPJ Web of Conferences , vol. 47 , EDP Sciences , Conference on Hot Planets and Cool Stars , Germany , 12/11/12 . https://doi.org/10.1051/epjconf/20134705007
dc.identifier.citationconference
dc.identifier.issn2100-014X
dc.identifier.otherORCID: /0000-0003-4600-5627/work/64327328
dc.identifier.urihttp://hdl.handle.net/2299/13927
dc.descriptionThis is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
dc.description.abstractIn order to compile a sample of ultracool dwarfs that will serve as benchmarks for testing theoretical formation and evolutionary models, we selected low-mass cool (>M7) objects that are potentially members of five known young Moving Groups in the solar neighbourhood. We have studied the kinematics of the sample, finding that 49 targets belong to the young disk area, from which 36 are kinematic member of one of the five moving groups under study. Some of the identified low-mass members have been spectroscopically characterised (T-eff, log g) and confirmed as young members through a detailed study of age indicators.en
dc.format.extent4
dc.format.extent169809
dc.language.isoeng
dc.publisherEDP Sciences
dc.relation.ispartofHot Planets and Cool Stars
dc.relation.ispartofseriesEPJ Web of Conferences
dc.subjectBROWN DWARFS
dc.subjectSTARS
dc.subjectSPECTROSCOPY
dc.subjectVELOCITIES
dc.subjectMEMBERS
dc.subjectSEARCH
dc.titleBenchmark low-mass objects in Moving Groupsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionScience & Technology Research Institute
rioxxterms.versionofrecord10.1051/epjconf/20134705007
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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