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- Publisher Website: 10.1111/j.1365-2966.2010.17660.x
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Article: A search for new members of the βPictoris, Tucana-Horologium and εCha moving groups in the RAVE data base
Title | A search for new members of the βPictoris, Tucana-Horologium and εCha moving groups in the RAVE data base |
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Authors | Kiss, László L.Moór, AttilaSzalai, TamásKovács, JózsefBayliss, Daniel D RGilmore, Gerard F.Bienaymé, OlivierBinney, James J.Bland-Hawthorn, Joss BlandCampbell, Randy D.Freeman, Kenneth C.Fulbright, Jon P.Gibson, Brad K.Grebel, Eva K.Helmi, AminaMunari, UlisseNavarro, Julio F.Parker, Quentin A.Reid, Warren A.Seabroke, George M.Siebert, ArnaudSiviero, AlessandroSteinmetz, MatthiasWatson, Fred G.Williams, Mary E KWyse, Rosemary F GZwitter, Tomaž |
Keywords | Open clusters and associations: individual: Tucana-Horologium association Stars: kinematics and dynamics Open clusters and associations: individual: εCha association Open clusters and associations: individual: β Pictoris moving group |
Issue Date | 2011 |
Citation | Monthly Notices of the Royal Astronomical Society, 2011, v. 411, n. 1, p. 117-123 How to Cite? |
Abstract | We report on the discovery of new members of nearby young moving groups, exploiting the full power of combining the Radial Velocity Experiment (RAVE) survey with several stellar age diagnostic methods and follow-up high-resolution optical spectroscopy. The results include the identification of one new and five likely members of the βPictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the εCha group and two stars in the Tucana-Horologium association. Based on the positive identifications, we foreshadow a great potential of the RAVE data base in progressing towards a full census of young moving groups in the solar neighbourhood. © 2010 The Authors. Journal compilation © 2010 RAS. |
Persistent Identifier | http://hdl.handle.net/10722/208919 |
ISSN | 2023 Impact Factor: 4.7 2023 SCImago Journal Rankings: 1.621 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Kiss, László L. | - |
dc.contributor.author | Moór, Attila | - |
dc.contributor.author | Szalai, Tamás | - |
dc.contributor.author | Kovács, József | - |
dc.contributor.author | Bayliss, Daniel D R | - |
dc.contributor.author | Gilmore, Gerard F. | - |
dc.contributor.author | Bienaymé, Olivier | - |
dc.contributor.author | Binney, James J. | - |
dc.contributor.author | Bland-Hawthorn, Joss Bland | - |
dc.contributor.author | Campbell, Randy D. | - |
dc.contributor.author | Freeman, Kenneth C. | - |
dc.contributor.author | Fulbright, Jon P. | - |
dc.contributor.author | Gibson, Brad K. | - |
dc.contributor.author | Grebel, Eva K. | - |
dc.contributor.author | Helmi, Amina | - |
dc.contributor.author | Munari, Ulisse | - |
dc.contributor.author | Navarro, Julio F. | - |
dc.contributor.author | Parker, Quentin A. | - |
dc.contributor.author | Reid, Warren A. | - |
dc.contributor.author | Seabroke, George M. | - |
dc.contributor.author | Siebert, Arnaud | - |
dc.contributor.author | Siviero, Alessandro | - |
dc.contributor.author | Steinmetz, Matthias | - |
dc.contributor.author | Watson, Fred G. | - |
dc.contributor.author | Williams, Mary E K | - |
dc.contributor.author | Wyse, Rosemary F G | - |
dc.contributor.author | Zwitter, Tomaž | - |
dc.date.accessioned | 2015-03-23T02:02:11Z | - |
dc.date.available | 2015-03-23T02:02:11Z | - |
dc.date.issued | 2011 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 2011, v. 411, n. 1, p. 117-123 | - |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.uri | http://hdl.handle.net/10722/208919 | - |
dc.description.abstract | We report on the discovery of new members of nearby young moving groups, exploiting the full power of combining the Radial Velocity Experiment (RAVE) survey with several stellar age diagnostic methods and follow-up high-resolution optical spectroscopy. The results include the identification of one new and five likely members of the βPictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the εCha group and two stars in the Tucana-Horologium association. Based on the positive identifications, we foreshadow a great potential of the RAVE data base in progressing towards a full census of young moving groups in the solar neighbourhood. © 2010 The Authors. Journal compilation © 2010 RAS. | - |
dc.language | eng | - |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | - |
dc.subject | Open clusters and associations: individual: Tucana-Horologium association | - |
dc.subject | Stars: kinematics and dynamics | - |
dc.subject | Open clusters and associations: individual: εCha association | - |
dc.subject | Open clusters and associations: individual: β Pictoris moving group | - |
dc.title | A search for new members of the βPictoris, Tucana-Horologium and εCha moving groups in the RAVE data base | - |
dc.type | Article | - |
dc.description.nature | link_to_OA_fulltext | - |
dc.identifier.doi | 10.1111/j.1365-2966.2010.17660.x | - |
dc.identifier.scopus | eid_2-s2.0-78751689898 | - |
dc.identifier.volume | 411 | - |
dc.identifier.issue | 1 | - |
dc.identifier.spage | 117 | - |
dc.identifier.epage | 123 | - |
dc.identifier.eissn | 1365-2966 | - |
dc.identifier.isi | WOS:000286525600024 | - |
dc.identifier.issnl | 0035-8711 | - |