Discovery of four field methane (T-type) dwarfs with the Two Micron All-Sky Survey

被引:180
作者
Burgasser, AJ
Kirkpatrick, JD
Brown, ME
Reid, IN
Gizis, JE
Dahn, CC
Monet, DG
Beichman, CA
Liebert, J
Cutri, RM
Skrutskie, MF
机构
[1] CALTECH, Div Phys, Pasadena, CA 91125 USA
[2] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA
[3] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[4] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[5] Univ Massachusetts, Five Coll Radio Astron Observ, Dept Phys & Astron, Dept Astron, Amherst, MA 01003 USA
[6] USN Observ, Flagstaff, AZ 86002 USA
[7] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[8] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
infrared : stars; stars : fundamental parameters; stars : individual (2MASSI J1047539+212423; 2MASSW J1217111-031113; 2MASSW; J1225543-273947; 2MASSW J1237392+652615; 2MASSW J1346464-003150); stars; low-mass; brown dwarfs;
D O I
10.1086/312221
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of four field methane ("T"-type) brown dwarfs using Two Micron All-Sky Survey (2MASS) data. One additional methane dwarf, previously discovered by the Sloan Digital Sky Survey, was also identified. Near-infrared spectra clearly show the 1.6 and 2.2 pm CH, absorption bands characteristic of objects with T-eff less than or similar to 1300 K as well as broadened H2O bands at 1.4 and 1.9 mu m. Comparing the spectra of these objects with that of Gl 229B, we propose that all new 2MASS T dwarfs are warmer than 950 K, in order from warmest to coolest: 2MASS J1217-03, 2MASS J1225-27, 2MASS J1047+21, and 2MASS J1237+65. Based on this preliminary sample, we find a warm T dwarf surface density of 0.0022 T dwarfs deg(-2), or similar to 90 warm T dwarfs over the whole sky detectable to J < 16. The resulting space density upper limit, 0.01 T dwarfs pc(-3), is comparable to that of the first L dwarf sample from Kirkpatrick et al.
引用
收藏
页码:L65 / L68
页数:4
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