Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey

被引:90
作者
Pinfield, D. J. [1 ]
Burningham, B. [1 ]
Tamura, M. [2 ]
Leggett, S. K. [3 ]
Lodieu, N. [4 ]
Lucas, P. W. [1 ]
Mortlock, D. J. [5 ]
Warren, S. J. [5 ]
Homeier, D. [6 ]
Ishii, M. [7 ]
Deacon, N. R. [8 ]
McMahon, R. G. [9 ]
Hewett, P. C. [9 ]
Osori, M. R. Zapatero [4 ]
Martin, E. L. [4 ]
Jones, H. R. A. [1 ]
Venemans, B. P. [9 ]
Day-Jones, A. C. [1 ]
Dobbie, P. D. [10 ]
Folkes, S. L. [1 ]
Dye, S. [11 ]
Allard, F. [12 ]
Baraffe, I. [13 ]
Barrado y Navascu, D. [14 ]
Casewell, S. L. [15 ]
Chiu, K. [16 ]
Chabrier, G. [13 ]
Clarke, F. [17 ]
Hodgkin, S. T. [9 ]
Magazzu, A. [18 ]
McCaughrean, M. J. [16 ]
Nakajima, T. [2 ]
Pavlenko, Y. [19 ]
Tinney, C. G. [20 ]
机构
[1] Univ Hertfordshire, Sci & Technol Res Inst, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England
[2] Natl Astron Observ, Mitaka, Tokyo 1818588, Japan
[3] Gemini Observ, Hilo, HI 96720 USA
[4] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Spain
[5] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England
[6] Georg August Univ, Inst Astrophys, D-37077 Gottingen, Germany
[7] Natl Inst Nat Sci, Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA
[8] Radboud Univ Nijmegen, Dept Astrophys, Fac Sci, NL-6500 GL Nijmegen, Netherlands
[9] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[10] Anglo Australian Observ, Epping, NSW 1710, Australia
[11] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales
[12] Univ Lyon, Ecole Normale Super, CNRS, UMR5574,Ctr Rech Astrophys Lyon, F-69364 Lyon, France
[13] Ecole Normale Super Lyon, CNRS, UMR 5574, CRAL, F-69364 Lyon, France
[14] INTA, Lab Astrofis Espacial & Fis Fundamental, E-2808 Madrid, Spain
[15] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[16] Univ Exeter, Sch Phys, Exeter EX4 4QL, Devon, England
[17] European So Observ, Santiago 19, Chile
[18] INAF, Fdn Galileo Galilei, E-38700 Santa Cruz De La Palma, Spain
[19] Natl Acad Sci, Main Astron Observ, UA-03680 Kiev 127, Ukraine
[20] Univ New S Wales, Dept Astrophys, Sydney, NSW 2052, Australia
基金
英国科学技术设施理事会; 美国国家航空航天局; 美国国家科学基金会;
关键词
techniques: photometric; techniques: spectroscopic; surveys; stars:; low-mass; brown dwarfs; infrared: stars;
D O I
10.1111/j.1365-2966.2008.13729.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the discovery of 15 new T2.5-T7.5 dwarfs (with estimated distances similar to 24-93 pc), identified in the first three main data releases of the United Kingdom Infrared Telescope (UKIRT) Infrared Deep Sky Survey. This brings the total number of T dwarfs discovered in the Large Area Survey (LAS) (to date) to 28. These discoveries are confirmed by near-infrared spectroscopy, from which we derive spectral types on the unified scheme of Burgasser et al. Seven of the new T dwarfs have spectral types of T2.5-T4.5, five have spectral types of T5-T5.5, one is a T6.5p and two are T7-7.5. We assess spectral morphology and colours to identify T dwarfs in our sample that may have non-typical physical properties (by comparison to solar neighbourhood populations), and find that three of these new T dwarfs may have unusual metallicity, two may have low surface gravity, and one may have high surface gravity. The colours of the full sample of LAS T dwarfs show a possible trend to bluer Y - J with decreasing effective temperature, and some interesting colour changes in J - H and z - J (deserving further investigation) beyond T8. The LAS T dwarf sample from the first and second main data releases show good evidence for a good level of completion to J = 19. By accounting for the main sources of incompleteness (selection, follow-up and spatial) as well as the effects of unresolved binarity, Malmquist and Eddington bias, we estimate that there are 17 +/- 4 >= T 4 dwarfs in the J <= 19 volume of the LAS second data release. This value is most consistent with theoretical predictions if the substellar mass function exponent alpha (dN/dm alpha m(-alpha)) lies between -1.0 and 0. This is consistent with the latest 2-Micron All Sky Survey (2MASS)/Sloan Digital Sky Survey (SDSS) constraint (which is based on lower number statistics) and is significantly lower than the alpha similar to 1.0 suggested by L dwarf field populations, which is possibly a result of the lower mass range probed by the T dwarf class.
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页码:304 / 322
页数:19
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