Mart′?n,E.L.,Basri,G.,Zapatero Osorio,M.R.,Rebolo,R.,&Garc′?a L′o pez,R.J.1998,ApJ,507,L41 Mart′?n,E.L.,Delfosse,X.,Basri,G.,Goldman,B.,Forveille,T.,&Zapattero Osorio,M.R.1999a,AJ,118, 2466
Mart′?n,E.L.,Brandner,W.,&Basri,G.1999b,Science,283,1718
Mart′?n,E.L.,Zapatero Osorio,M.R.,&Lehto,H.J.2001a,ApJ,557,822
Mart′?n,E.L.,Dougados,C.,Magnier,E.,M′e nard,F.,Magazz`u,A.,Cuillandre,J.-C.,&Delfosse,X.2001b, ApJ,561,195
Mart′?n,E.L.,&Bouy,H.2000,New A,7,595
McGovern,M.R.,Kirkpatrick J.D.,McLean,I.S.,Burgasser,A.J.,Prato,L.,Lowrance,P.J.2004,ApJ, 600,1020
McLean,I.S.,McGovern,M.R.,Burgasser,A.J.,Kirkpatrick,J.D.,Prato,L.,&Kim,S.S.2003,ApJ,596, 561
Mekkaden,M.V.1999,A&A,344,111
M′e nard,F.,Delfosse,X.,&Monin,J.-L.2002,A&A,396,L35
M′e nard,F.,&Delfosse,X.2004,in Semaine de l’Astrophysique Francaise.EdP-Sciences,Conf.Series,Eds.
062cfb8171fe910ef12df84dbes,D.Barret,T.Contini,F.Meynadier&L.Pagani,in press
Mohanty,S.,Basri,G.Shu,F.,Allard,F.,&Chabrier,G.2002,ApJ,571,469
Mohanty,S.,&Basri,G.2003,ApJ,583,451
Mokler,F.,&Stelzer,B.2002,A&A,391,1025
Natta,A.,&Testi,L.2001,A&A,376,L22
Pascucci,I.,Apai,D.,Henning,T.,&Dullemond,C.P.2003,ApJ,590,L111
Rebolo,R.,Mart′?n,E.L.,&Magazz`u,A.1992,ApJ,389,L83
Reid,I.N.,Kirkpatrick,J.D.,Gizis,J.E.,&Liebert,J.1999,ApJ,527,L105
Reid,I.N.,Kirkpatrick,J.D.,Gizis,J.E.,et al.2000,AJ,119,369
Ruiz,M.T.,Leggett,S.K.,&Allard,F.1997,ApJ,491,L107
S′a nchez-Lavega,A.2001,A&A,377,354
Schmidt,G.D.,Elston,R.,&Lupie,O.L.1992,AJ,104,1563
Schubert,G.,&Zhang,K.2000,in ASP Conf.Ser.212,From Giant Planets to Cool Stars,ed.C.A.Gri?th, M.S.Marley,(Flagsta?:ASP),210
Sengupta,S.,&Krishan,V.2001,ApJ,561,L123
Sengupta,S.2003,ApJ,585,L155
Simmons,J.F.L.,&Stewart,B.G.1985,A&A,142,100
–20–
Schweitzer,A.,Gizis,J.E.,Hauschildt,P.H.,Allard,F.,&Reid,I.N.2001,ApJ,555,368
Tamburini,F.,Ortolani,S.,&Bianchini,A.2002,A&A,394,675
Tsuji,T.,Ohnaka,K.,Aoki,W.,&Nakajima,T.1996,ApJ,308,L29
Tsuji,T.,Nakajima,T.,&Yanagisawa,K.2004,ApJ,607,511
Turnshek,D.A.,Bohlin,R.C.,Williamson,R.L.II,Lupie,O.L.,Koornneef,J.,&Morgan,D.H.1990,AJ, 99,1243
Vrba,F.J.,Henden,A.A.,Luginbuhl,C.B.,et al.2004,AJ,127,2948
Whittet,D.C.B.,Martin,P.G.,Hough,J.H.,Rouse,M.F.,Bailey,J.A.,&Axon,D.J.1992,ApJ,386,562 Wilson,J.C.,Miller,N.A.,Gizis,J.E.,et al.2003,in IAU Symposium211,Brown Dwarfs,ed.E.L.Mart′?n (San Francisco:ASP),197
Weitenbeck,A.J.2004,Acta Astron.,54,87
Woitke,P.,&Helling,Ch.2004,A&A,414,335
Zapatero Osorio,M.R.,Caballero,J.A.,B′e jar,V.J.S.,&Rebolo,R.2003,A&A,408,663
Zapatero Osorio,M.R.,&Mart′?n,E.L.2004,A&A,419,167
–21–
Fig. 1.—The Stokes parameters,Q/I and U/I,of our target sample are plotted against each other.All observations are in the Johnson I-band centred on850nm and150nm wide.Filled circles stand for the likely polarized dwarfs with detections at≥3σ.The mean values of J2158?15 and J2252?17are plotted as circled dots.Error bars of non-detections are avoided for the clarity of the?gure.
百度搜索“70edu”或“70教育网”即可找到本站免费阅读全部范文。收藏本站方便下次阅读,70教育网,提供经典行业范文Optical Linear Polarization of Late M- and L-Type Dwarfs(8)在线全文阅读。
相关推荐: