BANYAN. V. A SYSTEMATIC ALL-SKY SURVEY FOR NEW VERY LATE-TYPE LOW-MASS STARS AND BROWN DWARFS IN NEARBY YOUNG MOVING GROUPS

被引:102
作者
Gagne, Jonathan [1 ]
Lafreniere, David [1 ]
Doyon, Rene [1 ]
Malo, Lison [1 ,2 ]
Artigau, Etienne [1 ]
机构
[1] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada
[2] Canada France Hawaii Telescope, Kamuela, HI 96743 USA
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; methods: data analysis; proper motions; stars: kinematics and dynamics; stars: low-mass; VERY-LOW MASS; STELLAR KINEMATIC GROUPS; TW HYDRAE ASSOCIATION; VELOCITY EXPERIMENT RAVE; PROPER MOTION STARS; BETA-PICTORIS; RADIAL-VELOCITY; SOLAR NEIGHBORHOOD; TRIGONOMETRIC PARALLAXES; ULTRACOOL DWARFS;
D O I
10.1088/0004-637X/798/2/73
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the BANYAN All-Sky Survey (BASS) catalog, consisting of 228 new late-type (M4-L6) candidate members of nearby young moving groups (YMGs) with an expected false-positive rate of similar to 13%. This sample includes 79 new candidate young brown dwarfs and 22 planetary-mass objects. These candidates were identified through the first systematic all-sky survey for late-type low-mass stars and brown dwarfs in YMGs. We cross-matched the Two Micron All Sky Survey and AllWISE catalogs outside of the galactic plane to build a sample of 98,970 potential >= M5 dwarfs in the solar neighborhood and calculated their proper motions with typical precisions of 5-15 mas yr(-1). We selected highly probable candidate members of several YMGs from this sample using the Bayesian Analysis for Nearby Young AssociatioNs II tool (BANYAN II). We used the most probable statistical distances inferred from BANYAN II to estimate the spectral type and mass of these candidate YMG members. We used this unique sample to show tentative signs of mass segregation in the AB Doradus moving group and the Tucana-Horologium and Columba associations. The BASS sample has already been successful in identifying several new young brown dwarfs in earlier publications, and will be of great interest in studying the initial mass function of YMGs and for the search of exoplanets by direct imaging; the input sample of potential close-by >= M5 dwarfs will be useful to study the kinematics of low-mass stars and brown dwarfs and search for new proper motion pairs.
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页数:33
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共 205 条
  • [1] Allard F., 2013, MSAIS, V24, P128, DOI [10.48550/arXiv.1302.6559, DOI 10.48550/ARXIV.1302.6559]
  • [2] A new brown dwarf desert? A scarcity of wide ultracool binaries
    Allen, Peter R.
    Koerner, David W.
    McElwain, Michael W.
    Cruz, Kelle L.
    Reid, I. Neill
    [J]. ASTRONOMICAL JOURNAL, 2007, 133 (03) : 971 - 978
  • [3] A NEAR-INFRARED SPECTROSCOPIC STUDY OF YOUNG FIELD ULTRACOOL DWARFS
    Allers, K. N.
    Liu, Michael C.
    [J]. ASTROPHYSICAL JOURNAL, 2013, 772 (02)
  • [4] Using the minimum spanning tree to trace mass segregation
    Allison, Richard J.
    Goodwin, Simon P.
    Parker, Richard J.
    Portegies Zwart, Simon
    de Grijs, Richard
    Kouwenhoven, M. B. N.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 395 (03) : 1449 - 1454
  • [5] Alves de Oliveira C., 2012, ASTRON ASTROPHYS, V539, P151
  • [6] [Anonymous], A A
  • [7] [Anonymous], AJ
  • [8] Artigau É, 2009, AIP CONF PROC, V1094, P493, DOI 10.1063/1.3099156
  • [9] Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
    Baraffe, I
    Chabrier, G
    Barman, TS
    Allard, F
    Hauschildt, PH
    [J]. ASTRONOMY & ASTROPHYSICS, 2003, 402 (02) : 701 - 712
  • [10] A KINE-CHEMICAL INVESTIGATION OF THE AB DOR MOVING GROUP "STREAM"
    Barenfeld, Scott A.
    Bubar, Eric J.
    Mamajek, Eric E.
    Young, Patrick A.
    [J]. ASTROPHYSICAL JOURNAL, 2013, 766 (01)