A search for new members of they Pictoris, Tucana-Horologium and ∈ Cha moving groups in the RAVE data base
Identifieur interne : 002047 ( PascalFrancis/Corpus ); précédent : 002046; suivant : 002048A search for new members of they Pictoris, Tucana-Horologium and ∈ Cha moving groups in the RAVE data base
Auteurs : L. L. Kiss ; A. Moor ; T. Szalai ; J. Kovacs ; D. Bayliss ; G. F. Gilmore ; O. Bienayme ; J. Binney ; J. Bland-Hawthorn ; R. Campbell ; K. C. Freeman ; J. P. Fulbright ; B. K. Gibson ; E. K. Grebel ; A. Helmi ; U. Munari ; J. F. Navarro ; Q. A. Parker ; W. Reid ; G. M. Seabroke ; A. Siebert ; A. Siviero ; M. Steinmetz ; F. G. Watson ; M. Williams ; R. F. G. Wyse ; T. ZwitterSource :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011.
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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 β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ∈ Cha 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.
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Format Inist (serveur)
| NO : | PASCAL 11-0081152 INIST |
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| ET : | A search for new members of they Pictoris, Tucana-Horologium and ∈ Cha moving groups in the RAVE data base |
| AU : | KISS (L. L.); MOOR (A.); SZALAI (T.); KOVACS (J.); BAYLISS (D.); GILMORE (G. F.); BIENAYME (O.); BINNEY (J.); BLAND-HAWTHORN (J.); CAMPBELL (R.); FREEMAN (K. C.); FULBRIGHT (J. P.); GIBSON (B. K.); GREBEL (E. K.); HELMI (A.); MUNARI (U.); NAVARRO (J. F.); PARKER (Q. A.); REID (W.); SEABROKE (G. M.); SIEBERT (A.); SIVIERO (A.); STEINMETZ (M.); WATSON (F. G.); WILLIAMS (M.); WYSE (R. F. G.); ZWITTER (T.) |
| AF : | Konkoly Observatory of the Hungarian Academy of Sciences, PO Box 67/1525 Budapest/Hongrie (1 aut., 2 aut.); Sydney Institute for Astronomy, School of Physics, University of Sydney/NSW 2006/Australie (1 aut., 9 aut.); Department of Optics and Quantum Electronics, University of Szeged, Dóm tér 9./6720 Szeged/Hongrie (3 aut.); Gothard Astrophysical Observatory, ELTE University/9707 Szombathely/Hongrie (4 aut.); Research School of Astronomy and Astrophysics, The Australian National University/Canberra/Australie (5 aut., 11 aut.); Institute of Astronomy University of Cambridge, Madingley Road/Cambridge CB3 OHA/Royaume-Uni (6 aut.); Observatoire de Strasbourg, 11 Rue de L'Université/67000 Strasbourg/France (7 aut., 21 aut.); Rudolf Pierls Center,for Theoretical Physics, University of Oxford, 1 Keble Road/Oxford OX1 3NP/Royaume-Uni (8 aut.); Western Kentucky University/Bowling Green, Kentucky/Etats-Unis (10 aut.); Johns Hopkins University, 3400 N Charles Street/Baltimore, MD 21218/Etats-Unis (12 aut., 26 aut.); Jeremiah Horrocks Institute for Astrophysics & Supercomputing, University of Central Lancashire, Preston/Lancashire PR1 2HE/Royaume-Uni (13 aut.); Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg/69120 Heidelberg/Allemagne (14 aut.); Kapteyn Astronomical Institute, University of Groningen, Postbus 800/9700 AV Groningen/Pays-Bas (15 aut.); INAF Osservatorio Astronomico di Padova, Via dell 'Osservatorio 8/Asiago 36012/Italie (16 aut., 22 aut.); University of Victoria, PO Box 3055, Station CSC/Victoria, BC V8W 3P6/Canada (17 aut.); Macquarie University/Sydney, NSW 2109/Australie (18 aut., 19 aut.); Australian Astronomical Observatory, PO Box 296/Epping, NSW 1710/Australie (18 aut., 24 aut.); Mullard Space Science Laboratory, University College London, Holmbury St Mary/Dorking RH5 6NT/Royaume-Uni (20 aut.); Astrophysikalisches Institut Potsdam An der Sterwarte 16/14482 Potsdam/Allemagne (22 aut., 23 aut., 25 aut.); Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19/Ljubljana/Slovénie (27 aut.); Center of excellence SPACE-SI/Ljubljana/Slovénie (27 aut.) |
| DT : | Publication en série; Niveau analytique |
| SO : | Monthly Notices of the Royal Astronomical Society; ISSN 0035-8711; Coden MNRAA4; Etats-Unis; Da. 2011; Vol. 411; No. 1; Pp. 117-123; Bibl. 1/4 p. |
| LA : | Anglais |
| EA : | 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 β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ∈ Cha 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. |
| CC : | 001E03 |
| FD : | Vitesse radiale; Age; Spectrométrie optique; Type spectral; Voisinage solaire; Cinématique stellaire; Dynamique stellaire; Amas ouvert; Amas stellaire |
| ED : | Radial velocity; Age; Optical spectrometry; Spectral type; Solar neighborhood; Stellar kinematics; Stellar dynamics; Open clusters; Star clusters |
| SD : | Edad; Espectrometría óptica; Tipo espectral; Vecindad solar; Cinematica estelar |
| LO : | INIST-2067.354000193526170100 |
| ID : | 11-0081152 |
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Pascal:11-0081152Le document en format XML
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Binney</name><affiliation><inist:fA14 i1="08"><s1>Rudolf Pierls Center,for Theoretical Physics, University of Oxford, 1 Keble Road</s1><s2>Oxford OX1 3NP</s2><s3>GBR</s3><sZ>8 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Bland Hawthorn, J" sort="Bland Hawthorn, J" uniqKey="Bland Hawthorn J" first="J." last="Bland-Hawthorn">J. Bland-Hawthorn</name><affiliation><inist:fA14 i1="02"><s1>Sydney Institute for Astronomy, School of Physics, University of Sydney</s1><s2>NSW 2006</s2><s3>AUS</s3><sZ>1 aut.</sZ><sZ>9 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Campbell, R" sort="Campbell, R" uniqKey="Campbell R" first="R." last="Campbell">R. Campbell</name><affiliation><inist:fA14 i1="09"><s1>Western Kentucky University</s1><s2>Bowling Green, Kentucky</s2><s3>USA</s3><sZ>10 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Freeman, K C" sort="Freeman, K C" uniqKey="Freeman K" first="K. C." last="Freeman">K. C. Freeman</name><affiliation><inist:fA14 i1="05"><s1>Research School of Astronomy and Astrophysics, The Australian National University</s1><s2>Canberra</s2><s3>AUS</s3><sZ>5 aut.</sZ><sZ>11 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Fulbright, J P" sort="Fulbright, J P" uniqKey="Fulbright J" first="J. P." last="Fulbright">J. P. Fulbright</name><affiliation><inist:fA14 i1="10"><s1>Johns Hopkins University, 3400 N Charles Street</s1><s2>Baltimore, MD 21218</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>26 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Gibson, B K" sort="Gibson, B K" uniqKey="Gibson B" first="B. K." last="Gibson">B. K. Gibson</name><affiliation><inist:fA14 i1="11"><s1>Jeremiah Horrocks Institute for Astrophysics & Supercomputing, University of Central Lancashire, Preston</s1><s2>Lancashire PR1 2HE</s2><s3>GBR</s3><sZ>13 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Grebel, E K" sort="Grebel, E K" uniqKey="Grebel E" first="E. K." last="Grebel">E. K. Grebel</name><affiliation><inist:fA14 i1="12"><s1>Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg</s1><s2>69120 Heidelberg</s2><s3>DEU</s3><sZ>14 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Helmi, A" sort="Helmi, A" uniqKey="Helmi A" first="A." last="Helmi">A. Helmi</name><affiliation><inist:fA14 i1="13"><s1>Kapteyn Astronomical Institute, University of Groningen, Postbus 800</s1><s2>9700 AV Groningen</s2><s3>NLD</s3><sZ>15 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Munari, U" sort="Munari, U" uniqKey="Munari U" first="U." last="Munari">U. Munari</name><affiliation><inist:fA14 i1="14"><s1>INAF Osservatorio Astronomico di Padova, Via dell 'Osservatorio 8</s1><s2>Asiago 36012</s2><s3>ITA</s3><sZ>16 aut.</sZ><sZ>22 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Navarro, J F" sort="Navarro, J F" uniqKey="Navarro J" first="J. F." last="Navarro">J. F. Navarro</name><affiliation><inist:fA14 i1="15"><s1>University of Victoria, PO Box 3055, Station CSC</s1><s2>Victoria, BC V8W 3P6</s2><s3>CAN</s3><sZ>17 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Parker, Q A" sort="Parker, Q A" uniqKey="Parker Q" first="Q. A." last="Parker">Q. A. Parker</name><affiliation><inist:fA14 i1="16"><s1>Macquarie University</s1><s2>Sydney, NSW 2109</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>19 aut.</sZ></inist:fA14></affiliation><affiliation><inist:fA14 i1="17"><s1>Australian Astronomical Observatory, PO Box 296</s1><s2>Epping, NSW 1710</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>24 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Reid, W" sort="Reid, W" uniqKey="Reid W" first="W." last="Reid">W. Reid</name><affiliation><inist:fA14 i1="16"><s1>Macquarie University</s1><s2>Sydney, NSW 2109</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>19 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Seabroke, G M" sort="Seabroke, G M" uniqKey="Seabroke G" first="G. M." last="Seabroke">G. M. Seabroke</name><affiliation><inist:fA14 i1="18"><s1>Mullard Space Science Laboratory, University College London, Holmbury St Mary</s1><s2>Dorking RH5 6NT</s2><s3>GBR</s3><sZ>20 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Siebert, A" sort="Siebert, A" uniqKey="Siebert A" first="A." last="Siebert">A. Siebert</name><affiliation><inist:fA14 i1="07"><s1>Observatoire de Strasbourg, 11 Rue de L'Université</s1><s2>67000 Strasbourg</s2><s3>FRA</s3><sZ>7 aut.</sZ><sZ>21 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Siviero, A" sort="Siviero, A" uniqKey="Siviero A" first="A." last="Siviero">A. Siviero</name><affiliation><inist:fA14 i1="14"><s1>INAF Osservatorio Astronomico di Padova, Via dell 'Osservatorio 8</s1><s2>Asiago 36012</s2><s3>ITA</s3><sZ>16 aut.</sZ><sZ>22 aut.</sZ></inist:fA14></affiliation><affiliation><inist:fA14 i1="19"><s1>Astrophysikalisches Institut Potsdam An der Sterwarte 16</s1><s2>14482 Potsdam</s2><s3>DEU</s3><sZ>22 aut.</sZ><sZ>23 aut.</sZ><sZ>25 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Steinmetz, M" sort="Steinmetz, M" uniqKey="Steinmetz M" first="M." last="Steinmetz">M. Steinmetz</name><affiliation><inist:fA14 i1="19"><s1>Astrophysikalisches Institut Potsdam An der Sterwarte 16</s1><s2>14482 Potsdam</s2><s3>DEU</s3><sZ>22 aut.</sZ><sZ>23 aut.</sZ><sZ>25 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Watson, F G" sort="Watson, F G" uniqKey="Watson F" first="F. G." last="Watson">F. G. Watson</name><affiliation><inist:fA14 i1="17"><s1>Australian Astronomical Observatory, PO Box 296</s1><s2>Epping, NSW 1710</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>24 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Williams, M" sort="Williams, M" uniqKey="Williams M" first="M." last="Williams">M. Williams</name><affiliation><inist:fA14 i1="19"><s1>Astrophysikalisches Institut Potsdam An der Sterwarte 16</s1><s2>14482 Potsdam</s2><s3>DEU</s3><sZ>22 aut.</sZ><sZ>23 aut.</sZ><sZ>25 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Wyse, R F G" sort="Wyse, R F G" uniqKey="Wyse R" first="R. F. G." last="Wyse">R. F. G. Wyse</name><affiliation><inist:fA14 i1="10"><s1>Johns Hopkins University, 3400 N Charles Street</s1><s2>Baltimore, MD 21218</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>26 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Zwitter, T" sort="Zwitter, T" uniqKey="Zwitter T" first="T." last="Zwitter">T. Zwitter</name><affiliation><inist:fA14 i1="20"><s1>Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19</s1><s2>Ljubljana</s2><s3>SVN</s3><sZ>27 aut.</sZ></inist:fA14></affiliation><affiliation><inist:fA14 i1="21"><s1>Center of excellence SPACE-SI</s1><s2>Ljubljana</s2><s3>SVN</s3><sZ>27 aut.</sZ></inist:fA14></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">INIST</idno><idno type="inist">11-0081152</idno><date when="2011">2011</date><idno type="stanalyst">PASCAL 11-0081152 INIST</idno><idno type="RBID">Pascal:11-0081152</idno><idno type="wicri:Area/PascalFrancis/Corpus">002047</idno></publicationStmt><sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">A search for new members of they Pictoris, Tucana-Horologium and ∈ Cha moving groups in the RAVE data base</title><author><name sortKey="Kiss, L L" sort="Kiss, L L" uniqKey="Kiss L" first="L. L." last="Kiss">L. L. Kiss</name><affiliation><inist:fA14 i1="01"><s1>Konkoly Observatory of the Hungarian Academy of Sciences, PO Box 67</s1><s2>1525 Budapest</s2><s3>HUN</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ></inist:fA14></affiliation><affiliation><inist:fA14 i1="02"><s1>Sydney Institute for Astronomy, School of Physics, University of Sydney</s1><s2>NSW 2006</s2><s3>AUS</s3><sZ>1 aut.</sZ><sZ>9 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Moor, A" sort="Moor, A" uniqKey="Moor A" first="A." last="Moor">A. Moor</name><affiliation><inist:fA14 i1="01"><s1>Konkoly Observatory of the Hungarian Academy of Sciences, PO Box 67</s1><s2>1525 Budapest</s2><s3>HUN</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Szalai, T" sort="Szalai, T" uniqKey="Szalai T" first="T." last="Szalai">T. Szalai</name><affiliation><inist:fA14 i1="03"><s1>Department of Optics and Quantum Electronics, University of Szeged, Dóm tér 9.</s1><s2>6720 Szeged</s2><s3>HUN</s3><sZ>3 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Kovacs, J" sort="Kovacs, J" uniqKey="Kovacs J" first="J." last="Kovacs">J. Kovacs</name><affiliation><inist:fA14 i1="04"><s1>Gothard Astrophysical Observatory, ELTE University</s1><s2>9707 Szombathely</s2><s3>HUN</s3><sZ>4 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Bayliss, D" sort="Bayliss, D" uniqKey="Bayliss D" first="D." last="Bayliss">D. Bayliss</name><affiliation><inist:fA14 i1="05"><s1>Research School of Astronomy and Astrophysics, The Australian National University</s1><s2>Canberra</s2><s3>AUS</s3><sZ>5 aut.</sZ><sZ>11 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Gilmore, G F" sort="Gilmore, G F" uniqKey="Gilmore G" first="G. F." last="Gilmore">G. F. Gilmore</name><affiliation><inist:fA14 i1="06"><s1>Institute of Astronomy University of Cambridge, Madingley Road</s1><s2>Cambridge CB3 OHA</s2><s3>GBR</s3><sZ>6 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Bienayme, O" sort="Bienayme, O" uniqKey="Bienayme O" first="O." last="Bienayme">O. Bienayme</name><affiliation><inist:fA14 i1="07"><s1>Observatoire de Strasbourg, 11 Rue de L'Université</s1><s2>67000 Strasbourg</s2><s3>FRA</s3><sZ>7 aut.</sZ><sZ>21 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Binney, J" sort="Binney, J" uniqKey="Binney J" first="J." last="Binney">J. Binney</name><affiliation><inist:fA14 i1="08"><s1>Rudolf Pierls Center,for Theoretical Physics, University of Oxford, 1 Keble Road</s1><s2>Oxford OX1 3NP</s2><s3>GBR</s3><sZ>8 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Bland Hawthorn, J" sort="Bland Hawthorn, J" uniqKey="Bland Hawthorn J" first="J." last="Bland-Hawthorn">J. Bland-Hawthorn</name><affiliation><inist:fA14 i1="02"><s1>Sydney Institute for Astronomy, School of Physics, University of Sydney</s1><s2>NSW 2006</s2><s3>AUS</s3><sZ>1 aut.</sZ><sZ>9 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Campbell, R" sort="Campbell, R" uniqKey="Campbell R" first="R." last="Campbell">R. Campbell</name><affiliation><inist:fA14 i1="09"><s1>Western Kentucky University</s1><s2>Bowling Green, Kentucky</s2><s3>USA</s3><sZ>10 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Freeman, K C" sort="Freeman, K C" uniqKey="Freeman K" first="K. C." last="Freeman">K. C. Freeman</name><affiliation><inist:fA14 i1="05"><s1>Research School of Astronomy and Astrophysics, The Australian National University</s1><s2>Canberra</s2><s3>AUS</s3><sZ>5 aut.</sZ><sZ>11 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Fulbright, J P" sort="Fulbright, J P" uniqKey="Fulbright J" first="J. P." last="Fulbright">J. P. Fulbright</name><affiliation><inist:fA14 i1="10"><s1>Johns Hopkins University, 3400 N Charles Street</s1><s2>Baltimore, MD 21218</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>26 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Gibson, B K" sort="Gibson, B K" uniqKey="Gibson B" first="B. K." last="Gibson">B. K. Gibson</name><affiliation><inist:fA14 i1="11"><s1>Jeremiah Horrocks Institute for Astrophysics & Supercomputing, University of Central Lancashire, Preston</s1><s2>Lancashire PR1 2HE</s2><s3>GBR</s3><sZ>13 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Grebel, E K" sort="Grebel, E K" uniqKey="Grebel E" first="E. K." last="Grebel">E. K. Grebel</name><affiliation><inist:fA14 i1="12"><s1>Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg</s1><s2>69120 Heidelberg</s2><s3>DEU</s3><sZ>14 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Helmi, A" sort="Helmi, A" uniqKey="Helmi A" first="A." last="Helmi">A. Helmi</name><affiliation><inist:fA14 i1="13"><s1>Kapteyn Astronomical Institute, University of Groningen, Postbus 800</s1><s2>9700 AV Groningen</s2><s3>NLD</s3><sZ>15 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Munari, U" sort="Munari, U" uniqKey="Munari U" first="U." last="Munari">U. Munari</name><affiliation><inist:fA14 i1="14"><s1>INAF Osservatorio Astronomico di Padova, Via dell 'Osservatorio 8</s1><s2>Asiago 36012</s2><s3>ITA</s3><sZ>16 aut.</sZ><sZ>22 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Navarro, J F" sort="Navarro, J F" uniqKey="Navarro J" first="J. F." last="Navarro">J. F. Navarro</name><affiliation><inist:fA14 i1="15"><s1>University of Victoria, PO Box 3055, Station CSC</s1><s2>Victoria, BC V8W 3P6</s2><s3>CAN</s3><sZ>17 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Parker, Q A" sort="Parker, Q A" uniqKey="Parker Q" first="Q. A." last="Parker">Q. A. Parker</name><affiliation><inist:fA14 i1="16"><s1>Macquarie University</s1><s2>Sydney, NSW 2109</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>19 aut.</sZ></inist:fA14></affiliation><affiliation><inist:fA14 i1="17"><s1>Australian Astronomical Observatory, PO Box 296</s1><s2>Epping, NSW 1710</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>24 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Reid, W" sort="Reid, W" uniqKey="Reid W" first="W." last="Reid">W. Reid</name><affiliation><inist:fA14 i1="16"><s1>Macquarie University</s1><s2>Sydney, NSW 2109</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>19 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Seabroke, G M" sort="Seabroke, G M" uniqKey="Seabroke G" first="G. M." last="Seabroke">G. M. Seabroke</name><affiliation><inist:fA14 i1="18"><s1>Mullard Space Science Laboratory, University College London, Holmbury St Mary</s1><s2>Dorking RH5 6NT</s2><s3>GBR</s3><sZ>20 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Siebert, A" sort="Siebert, A" uniqKey="Siebert A" first="A." last="Siebert">A. Siebert</name><affiliation><inist:fA14 i1="07"><s1>Observatoire de Strasbourg, 11 Rue de L'Université</s1><s2>67000 Strasbourg</s2><s3>FRA</s3><sZ>7 aut.</sZ><sZ>21 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Siviero, A" sort="Siviero, A" uniqKey="Siviero A" first="A." last="Siviero">A. Siviero</name><affiliation><inist:fA14 i1="14"><s1>INAF Osservatorio Astronomico di Padova, Via dell 'Osservatorio 8</s1><s2>Asiago 36012</s2><s3>ITA</s3><sZ>16 aut.</sZ><sZ>22 aut.</sZ></inist:fA14></affiliation><affiliation><inist:fA14 i1="19"><s1>Astrophysikalisches Institut Potsdam An der Sterwarte 16</s1><s2>14482 Potsdam</s2><s3>DEU</s3><sZ>22 aut.</sZ><sZ>23 aut.</sZ><sZ>25 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Steinmetz, M" sort="Steinmetz, M" uniqKey="Steinmetz M" first="M." last="Steinmetz">M. Steinmetz</name><affiliation><inist:fA14 i1="19"><s1>Astrophysikalisches Institut Potsdam An der Sterwarte 16</s1><s2>14482 Potsdam</s2><s3>DEU</s3><sZ>22 aut.</sZ><sZ>23 aut.</sZ><sZ>25 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Watson, F G" sort="Watson, F G" uniqKey="Watson F" first="F. G." last="Watson">F. G. Watson</name><affiliation><inist:fA14 i1="17"><s1>Australian Astronomical Observatory, PO Box 296</s1><s2>Epping, NSW 1710</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>24 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Williams, M" sort="Williams, M" uniqKey="Williams M" first="M." last="Williams">M. Williams</name><affiliation><inist:fA14 i1="19"><s1>Astrophysikalisches Institut Potsdam An der Sterwarte 16</s1><s2>14482 Potsdam</s2><s3>DEU</s3><sZ>22 aut.</sZ><sZ>23 aut.</sZ><sZ>25 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Wyse, R F G" sort="Wyse, R F G" uniqKey="Wyse R" first="R. F. G." last="Wyse">R. F. G. Wyse</name><affiliation><inist:fA14 i1="10"><s1>Johns Hopkins University, 3400 N Charles Street</s1><s2>Baltimore, MD 21218</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>26 aut.</sZ></inist:fA14></affiliation></author><author><name sortKey="Zwitter, T" sort="Zwitter, T" uniqKey="Zwitter T" first="T." last="Zwitter">T. Zwitter</name><affiliation><inist:fA14 i1="20"><s1>Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19</s1><s2>Ljubljana</s2><s3>SVN</s3><sZ>27 aut.</sZ></inist:fA14></affiliation><affiliation><inist:fA14 i1="21"><s1>Center of excellence SPACE-SI</s1><s2>Ljubljana</s2><s3>SVN</s3><sZ>27 aut.</sZ></inist:fA14></affiliation></author></analytic><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title><idno type="ISSN">0035-8711</idno><imprint><date when="2011">2011</date></imprint></series></biblStruct></sourceDesc><seriesStmt><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Age</term><term>Open clusters</term><term>Optical spectrometry</term><term>Radial velocity</term><term>Solar neighborhood</term><term>Spectral type</term><term>Star clusters</term><term>Stellar dynamics</term><term>Stellar kinematics</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Vitesse radiale</term><term>Age</term><term>Spectrométrie optique</term><term>Type spectral</term><term>Voisinage solaire</term><term>Cinématique stellaire</term><term>Dynamique stellaire</term><term>Amas ouvert</term><term>Amas stellaire</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">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 β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ∈ Cha 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.</div></front></TEI><inist><standard h6="B"><pA><fA01 i1="01" i2="1"><s0>0035-8711</s0></fA01><fA02 i1="01"><s0>MNRAA4</s0></fA02><fA03 i2="1"><s0>Mon. Not. R. Astron. Soc.</s0></fA03><fA05><s2>411</s2></fA05><fA06><s2>1</s2></fA06><fA08 i1="01" i2="1" l="ENG"><s1>A search for new members of they Pictoris, Tucana-Horologium and ∈ Cha moving groups in the RAVE data base</s1></fA08><fA11 i1="01" i2="1"><s1>KISS (L. L.)</s1></fA11><fA11 i1="02" i2="1"><s1>MOOR (A.)</s1></fA11><fA11 i1="03" i2="1"><s1>SZALAI (T.)</s1></fA11><fA11 i1="04" i2="1"><s1>KOVACS (J.)</s1></fA11><fA11 i1="05" i2="1"><s1>BAYLISS (D.)</s1></fA11><fA11 i1="06" i2="1"><s1>GILMORE (G. F.)</s1></fA11><fA11 i1="07" i2="1"><s1>BIENAYME (O.)</s1></fA11><fA11 i1="08" i2="1"><s1>BINNEY (J.)</s1></fA11><fA11 i1="09" i2="1"><s1>BLAND-HAWTHORN (J.)</s1></fA11><fA11 i1="10" i2="1"><s1>CAMPBELL (R.)</s1></fA11><fA11 i1="11" i2="1"><s1>FREEMAN (K. C.)</s1></fA11><fA11 i1="12" i2="1"><s1>FULBRIGHT (J. P.)</s1></fA11><fA11 i1="13" i2="1"><s1>GIBSON (B. K.)</s1></fA11><fA11 i1="14" i2="1"><s1>GREBEL (E. K.)</s1></fA11><fA11 i1="15" i2="1"><s1>HELMI (A.)</s1></fA11><fA11 i1="16" i2="1"><s1>MUNARI (U.)</s1></fA11><fA11 i1="17" i2="1"><s1>NAVARRO (J. F.)</s1></fA11><fA11 i1="18" i2="1"><s1>PARKER (Q. A.)</s1></fA11><fA11 i1="19" i2="1"><s1>REID (W.)</s1></fA11><fA11 i1="20" i2="1"><s1>SEABROKE (G. M.)</s1></fA11><fA11 i1="21" i2="1"><s1>SIEBERT (A.)</s1></fA11><fA11 i1="22" i2="1"><s1>SIVIERO (A.)</s1></fA11><fA11 i1="23" i2="1"><s1>STEINMETZ (M.)</s1></fA11><fA11 i1="24" i2="1"><s1>WATSON (F. G.)</s1></fA11><fA11 i1="25" i2="1"><s1>WILLIAMS (M.)</s1></fA11><fA11 i1="26" i2="1"><s1>WYSE (R. F. G.)</s1></fA11><fA11 i1="27" i2="1"><s1>ZWITTER (T.)</s1></fA11><fA14 i1="01"><s1>Konkoly Observatory of the Hungarian Academy of Sciences, PO Box 67</s1><s2>1525 Budapest</s2><s3>HUN</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ></fA14><fA14 i1="02"><s1>Sydney Institute for Astronomy, School of Physics, University of Sydney</s1><s2>NSW 2006</s2><s3>AUS</s3><sZ>1 aut.</sZ><sZ>9 aut.</sZ></fA14><fA14 i1="03"><s1>Department of Optics and Quantum Electronics, University of Szeged, Dóm tér 9.</s1><s2>6720 Szeged</s2><s3>HUN</s3><sZ>3 aut.</sZ></fA14><fA14 i1="04"><s1>Gothard Astrophysical Observatory, ELTE University</s1><s2>9707 Szombathely</s2><s3>HUN</s3><sZ>4 aut.</sZ></fA14><fA14 i1="05"><s1>Research School of Astronomy and Astrophysics, The Australian National University</s1><s2>Canberra</s2><s3>AUS</s3><sZ>5 aut.</sZ><sZ>11 aut.</sZ></fA14><fA14 i1="06"><s1>Institute of Astronomy University of Cambridge, Madingley Road</s1><s2>Cambridge CB3 OHA</s2><s3>GBR</s3><sZ>6 aut.</sZ></fA14><fA14 i1="07"><s1>Observatoire de Strasbourg, 11 Rue de L'Université</s1><s2>67000 Strasbourg</s2><s3>FRA</s3><sZ>7 aut.</sZ><sZ>21 aut.</sZ></fA14><fA14 i1="08"><s1>Rudolf Pierls Center,for Theoretical Physics, University of Oxford, 1 Keble Road</s1><s2>Oxford OX1 3NP</s2><s3>GBR</s3><sZ>8 aut.</sZ></fA14><fA14 i1="09"><s1>Western Kentucky University</s1><s2>Bowling Green, Kentucky</s2><s3>USA</s3><sZ>10 aut.</sZ></fA14><fA14 i1="10"><s1>Johns Hopkins University, 3400 N Charles Street</s1><s2>Baltimore, MD 21218</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>26 aut.</sZ></fA14><fA14 i1="11"><s1>Jeremiah Horrocks Institute for Astrophysics & Supercomputing, University of Central Lancashire, Preston</s1><s2>Lancashire PR1 2HE</s2><s3>GBR</s3><sZ>13 aut.</sZ></fA14><fA14 i1="12"><s1>Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg</s1><s2>69120 Heidelberg</s2><s3>DEU</s3><sZ>14 aut.</sZ></fA14><fA14 i1="13"><s1>Kapteyn Astronomical Institute, University of Groningen, Postbus 800</s1><s2>9700 AV Groningen</s2><s3>NLD</s3><sZ>15 aut.</sZ></fA14><fA14 i1="14"><s1>INAF Osservatorio Astronomico di Padova, Via dell 'Osservatorio 8</s1><s2>Asiago 36012</s2><s3>ITA</s3><sZ>16 aut.</sZ><sZ>22 aut.</sZ></fA14><fA14 i1="15"><s1>University of Victoria, PO Box 3055, Station CSC</s1><s2>Victoria, BC V8W 3P6</s2><s3>CAN</s3><sZ>17 aut.</sZ></fA14><fA14 i1="16"><s1>Macquarie University</s1><s2>Sydney, NSW 2109</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>19 aut.</sZ></fA14><fA14 i1="17"><s1>Australian Astronomical Observatory, PO Box 296</s1><s2>Epping, NSW 1710</s2><s3>AUS</s3><sZ>18 aut.</sZ><sZ>24 aut.</sZ></fA14><fA14 i1="18"><s1>Mullard Space Science Laboratory, University College London, Holmbury St Mary</s1><s2>Dorking RH5 6NT</s2><s3>GBR</s3><sZ>20 aut.</sZ></fA14><fA14 i1="19"><s1>Astrophysikalisches Institut Potsdam An der Sterwarte 16</s1><s2>14482 Potsdam</s2><s3>DEU</s3><sZ>22 aut.</sZ><sZ>23 aut.</sZ><sZ>25 aut.</sZ></fA14><fA14 i1="20"><s1>Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19</s1><s2>Ljubljana</s2><s3>SVN</s3><sZ>27 aut.</sZ></fA14><fA14 i1="21"><s1>Center of excellence SPACE-SI</s1><s2>Ljubljana</s2><s3>SVN</s3><sZ>27 aut.</sZ></fA14><fA20><s1>117-123</s1></fA20><fA21><s1>2011</s1></fA21><fA23 i1="01"><s0>ENG</s0></fA23><fA43 i1="01"><s1>INIST</s1><s2>2067</s2><s5>354000193526170100</s5></fA43><fA44><s0>0000</s0><s1>© 2011 INIST-CNRS. All rights reserved.</s1></fA44><fA45><s0>1/4 p.</s0></fA45><fA47 i1="01" i2="1"><s0>11-0081152</s0></fA47><fA60><s1>P</s1></fA60><fA61><s0>A</s0></fA61><fA64 i1="01" i2="1"><s0>Monthly Notices of the Royal Astronomical Society</s0></fA64><fA66 i1="01"><s0>USA</s0></fA66><fC01 i1="01" l="ENG"><s0>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 β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ∈ Cha 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.</s0></fC01><fC02 i1="01" i2="3"><s0>001E03</s0></fC02><fC03 i1="01" i2="3" l="FRE"><s0>Vitesse radiale</s0><s5>26</s5></fC03><fC03 i1="01" i2="3" l="ENG"><s0>Radial velocity</s0><s5>26</s5></fC03><fC03 i1="02" i2="X" l="FRE"><s0>Age</s0><s5>27</s5></fC03><fC03 i1="02" i2="X" l="ENG"><s0>Age</s0><s5>27</s5></fC03><fC03 i1="02" i2="X" l="SPA"><s0>Edad</s0><s5>27</s5></fC03><fC03 i1="03" i2="X" l="FRE"><s0>Spectrométrie optique</s0><s5>28</s5></fC03><fC03 i1="03" i2="X" l="ENG"><s0>Optical spectrometry</s0><s5>28</s5></fC03><fC03 i1="03" i2="X" l="SPA"><s0>Espectrometría óptica</s0><s5>28</s5></fC03><fC03 i1="04" i2="X" l="FRE"><s0>Type spectral</s0><s5>29</s5></fC03><fC03 i1="04" i2="X" l="ENG"><s0>Spectral type</s0><s5>29</s5></fC03><fC03 i1="04" i2="X" l="SPA"><s0>Tipo espectral</s0><s5>29</s5></fC03><fC03 i1="05" i2="X" l="FRE"><s0>Voisinage solaire</s0><s5>30</s5></fC03><fC03 i1="05" i2="X" l="ENG"><s0>Solar neighborhood</s0><s5>30</s5></fC03><fC03 i1="05" i2="X" l="SPA"><s0>Vecindad solar</s0><s5>30</s5></fC03><fC03 i1="06" i2="X" l="FRE"><s0>Cinématique stellaire</s0><s5>31</s5></fC03><fC03 i1="06" i2="X" l="ENG"><s0>Stellar kinematics</s0><s5>31</s5></fC03><fC03 i1="06" i2="X" l="SPA"><s0>Cinematica estelar</s0><s5>31</s5></fC03><fC03 i1="07" i2="3" l="FRE"><s0>Dynamique stellaire</s0><s5>32</s5></fC03><fC03 i1="07" i2="3" l="ENG"><s0>Stellar dynamics</s0><s5>32</s5></fC03><fC03 i1="08" i2="3" l="FRE"><s0>Amas ouvert</s0><s5>33</s5></fC03><fC03 i1="08" i2="3" l="ENG"><s0>Open clusters</s0><s5>33</s5></fC03><fC03 i1="09" i2="3" l="FRE"><s0>Amas stellaire</s0><s5>34</s5></fC03><fC03 i1="09" i2="3" l="ENG"><s0>Star clusters</s0><s5>34</s5></fC03><fN21><s1>052</s1></fN21><fN44 i1="01"><s1>OTO</s1></fN44><fN82><s1>OTO</s1></fN82></pA></standard><server><NO>PASCAL 11-0081152 INIST</NO><ET>A search for new members of they Pictoris, Tucana-Horologium and ∈ Cha moving groups in the RAVE data base</ET><AU>KISS (L. L.); MOOR (A.); SZALAI (T.); KOVACS (J.); BAYLISS (D.); GILMORE (G. F.); BIENAYME (O.); BINNEY (J.); BLAND-HAWTHORN (J.); CAMPBELL (R.); FREEMAN (K. C.); FULBRIGHT (J. P.); GIBSON (B. K.); GREBEL (E. K.); HELMI (A.); MUNARI (U.); NAVARRO (J. F.); PARKER (Q. A.); REID (W.); SEABROKE (G. M.); SIEBERT (A.); SIVIERO (A.); STEINMETZ (M.); WATSON (F. G.); WILLIAMS (M.); WYSE (R. F. G.); ZWITTER (T.)</AU><AF>Konkoly Observatory of the Hungarian Academy of Sciences, PO Box 67/1525 Budapest/Hongrie (1 aut., 2 aut.); Sydney Institute for Astronomy, School of Physics, University of Sydney/NSW 2006/Australie (1 aut., 9 aut.); Department of Optics and Quantum Electronics, University of Szeged, Dóm tér 9./6720 Szeged/Hongrie (3 aut.); Gothard Astrophysical Observatory, ELTE University/9707 Szombathely/Hongrie (4 aut.); Research School of Astronomy and Astrophysics, The Australian National University/Canberra/Australie (5 aut., 11 aut.); Institute of Astronomy University of Cambridge, Madingley Road/Cambridge CB3 OHA/Royaume-Uni (6 aut.); Observatoire de Strasbourg, 11 Rue de L'Université/67000 Strasbourg/France (7 aut., 21 aut.); Rudolf Pierls Center,for Theoretical Physics, University of Oxford, 1 Keble Road/Oxford OX1 3NP/Royaume-Uni (8 aut.); Western Kentucky University/Bowling Green, Kentucky/Etats-Unis (10 aut.); Johns Hopkins University, 3400 N Charles Street/Baltimore, MD 21218/Etats-Unis (12 aut., 26 aut.); Jeremiah Horrocks Institute for Astrophysics & Supercomputing, University of Central Lancashire, Preston/Lancashire PR1 2HE/Royaume-Uni (13 aut.); Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg/69120 Heidelberg/Allemagne (14 aut.); Kapteyn Astronomical Institute, University of Groningen, Postbus 800/9700 AV Groningen/Pays-Bas (15 aut.); INAF Osservatorio Astronomico di Padova, Via dell 'Osservatorio 8/Asiago 36012/Italie (16 aut., 22 aut.); University of Victoria, PO Box 3055, Station CSC/Victoria, BC V8W 3P6/Canada (17 aut.); Macquarie University/Sydney, NSW 2109/Australie (18 aut., 19 aut.); Australian Astronomical Observatory, PO Box 296/Epping, NSW 1710/Australie (18 aut., 24 aut.); Mullard Space Science Laboratory, University College London, Holmbury St Mary/Dorking RH5 6NT/Royaume-Uni (20 aut.); Astrophysikalisches Institut Potsdam An der Sterwarte 16/14482 Potsdam/Allemagne (22 aut., 23 aut., 25 aut.); Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19/Ljubljana/Slovénie (27 aut.); Center of excellence SPACE-SI/Ljubljana/Slovénie (27 aut.)</AF><DT>Publication en série; Niveau analytique</DT><SO>Monthly Notices of the Royal Astronomical Society; ISSN 0035-8711; Coden MNRAA4; Etats-Unis; Da. 2011; Vol. 411; No. 1; Pp. 117-123; Bibl. 1/4 p.</SO><LA>Anglais</LA><EA>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 β Pictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the ∈ Cha 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.</EA><CC>001E03</CC><FD>Vitesse radiale; Age; Spectrométrie optique; Type spectral; Voisinage solaire; Cinématique stellaire; Dynamique stellaire; Amas ouvert; Amas stellaire</FD><ED>Radial velocity; Age; Optical spectrometry; Spectral type; Solar neighborhood; Stellar kinematics; Stellar dynamics; Open clusters; Star clusters</ED><SD>Edad; Espectrometría óptica; Tipo espectral; Vecindad solar; Cinematica estelar</SD><LO>INIST-2067.354000193526170100</LO><ID>11-0081152</ID></server></inist></record>Pour manipuler ce document sous Unix (Dilib)
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