BANYAN. VI. DISCOVERY OF A COMPANION AT THE BROWN DWARF/PLANET-MASS LIMIT TO A TUCANA-HOROLOGIUM M DWARF

被引:36
作者
Artigau, Etienne [1 ]
Gagne, Jonathan [1 ]
Faherty, Jacqueline [2 ]
Malo, Lison [3 ]
Naud, Marie-Eve [1 ]
Doyon, Rene [1 ]
Lafreniere, David [1 ]
Beletsky, Yuri [4 ]
机构
[1] Univ Montreal, Dept Phys, Inst Rech Exoplanetes IREx, Montreal, PQ H3C 3J7, Canada
[2] Carnegie Inst Sci, Dept Terr Magnetism, Washington, DC 20015 USA
[3] Canada France Hawaii Telescope Corp, Kamuela, HI 96743 USA
[4] Carnegie Inst Sci, Las Campanas Observ, La Serena, Chile
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
brown dwarfs; stars: late-type; stars: low-mass; VERY-LOW MASS; LITHIUM DEPLETION BOUNDARY; GIANT PLANET FORMATION; STAR CANDIDATES; T-DWARFS; KINEMATIC GROUPS; BETA-PICTORIS; NEARBY STARS; YOUNG STARS; LOW-GRAVITY;
D O I
10.1088/0004-637X/806/2/254
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a substellar companion to 2MASS J02192210-3925225, a young M6. candidate member of the Tucana-Horologium association (30-40 Myr). This L4 gamma companion has been discovered with seeing-limited direct imaging observations; at a 4 '' separation (160 AU) and a modest contrast ratio, it joins the very short list of young low-mass companions amenable to study without the aid of adaptive optics, enabling its characterization with a much wider suite of instruments than is possible for companions uncovered by highcontrast imaging surveys. With a model-dependent mass of 12-15 M-Jup, it straddles the boundary between the planet and brown dwarf mass regimes. We present near-infrared spectroscopy of this companion and compare it to various similar objects uncovered in the last few years. The J0219-3925 system falls in a sparsely populated part of the host mass versus mass ratio diagram for binaries; the dearth of known similar companions may be due to observational biases in previous low-mass companion searches.
引用
收藏
页数:11
相关论文
共 81 条
[1]   Models of giant planet formation with migration and disc evolution [J].
Alibert, Y ;
Mordasini, C ;
Benz, W ;
Winisdoerffer, C .
ASTRONOMY & ASTROPHYSICS, 2005, 434 (01) :343-353
[2]  
Allard F., 2014, P IAU S, P271
[3]   A NEAR-INFRARED SPECTROSCOPIC STUDY OF YOUNG FIELD ULTRACOOL DWARFS [J].
Allers, K. N. ;
Liu, Michael C. .
ASTROPHYSICAL JOURNAL, 2013, 772 (02)
[4]  
Baraffe I, 1998, ASTRON ASTROPHYS, V337, P403
[5]   DISCOVERY AND CHARACTERIZATION OF WIDE BINARY SYSTEMS WITH A VERY LOW MASS COMPONENT [J].
Baron, Frederique ;
Lafreniere, David ;
Artigau, Etienne ;
Doyon, Rene ;
Gagne, Jonathan ;
Davison, Cassy L. ;
Malo, Lison ;
Robert, Jasmin ;
Nadeau, Daniel ;
Reyle, Celine .
ASTROPHYSICAL JOURNAL, 2015, 802 (01)
[6]   Imaging Young Giant Planets From Ground and Space [J].
Beichman, Charles A. ;
Krist, John ;
Trauger, John T. ;
Greene, Tom ;
Oppenheimer, Ben ;
Sivaramakrishnan, Anand ;
Doyon, Rene ;
Boccaletti, Anthony ;
Barman, Travis S. ;
Rieke, Marcia .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2010, 122 (888) :162-200
[7]   THE GEMINI/NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF PLANETS AROUND YOUNG MOVING GROUP STARS [J].
Biller, Beth A. ;
Liu, Michael C. ;
Wahhaj, Zahed ;
Nielsen, Eric L. ;
Hayward, Thomas L. ;
Males, Jared R. ;
Skemer, Andrew ;
Close, Laird M. ;
Chun, Mark ;
Ftaclas, Christ ;
Clarke, Fraser ;
Thatte, Niranjan ;
Shkolnik, Evgenya L. ;
Reid, I. Neill ;
Hartung, Markus ;
Boss, Alan ;
Lin, Douglas ;
Alencar, Silvia H. P. ;
Dal Pino, Elisabete de Gouveia ;
Gregorio-Hetem, Jane ;
Toomey, Douglas .
ASTROPHYSICAL JOURNAL, 2013, 777 (02)
[8]   A lithium depletion boundary age of 21 Myr for the Beta Pictoris moving group [J].
Binks, A. S. ;
Jeffries, R. D. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2014, 438 (01) :L11-L15
[9]   A library of near-infrared integral field spectra of young M-L dwarfs [J].
Bonnefoy, M. ;
Chauvin, G. ;
Lagrange, A. -M. ;
Rojo, P. ;
Allard, F. ;
Pinte, C. ;
Dumas, C. ;
Homeier, D. .
ASTRONOMY & ASTROPHYSICS, 2014, 562
[10]   Giant planet formation by gravitational instability [J].
Boss, AP .
SCIENCE, 1997, 276 (5320) :1836-1839