COLORS AND KINEMATICS OF L DWARFS FROM THE SLOAN DIGITAL SKY SURVEY

被引:146
作者
Schmidt, Sarah J. [1 ]
West, Andrew A. [2 ,3 ]
Hawley, Suzanne L. [1 ]
Pineda, J. Sebastian [2 ]
机构
[1] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[2] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
[3] Boston Univ, Dept Astron, Boston, MA 02215 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
brown dwarfs; solar neighborhood; stars: kinematics and dynamics; stars: low-mass; PROPER-MOTION SURVEY; EARLY DATA RELEASE; L FIELD DWARFS; BLUE L DWARF; T-DWARFS; ULTRACOOL DWARFS; COOL NEIGHBORS; MAIN-SEQUENCE; SPECTRAL CLASSIFICATION; LUMINOSITY FUNCTION;
D O I
10.1088/0004-6256/139/5/1808
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a sample of 484 L dwarfs, 210 of which are newly discovered from the Sloan Digital Sky Survey (SDSS) Data Release 7 spectroscopic database. We combine this sample with known L dwarfs to investigate their izJHK(S) colors. Our spectroscopically selected sample has similar to 0.1 mag bluer median J - K(S) color at a given spectral type (for L0-L4) than previously known L dwarfs, which reflects a bias toward redder L dwarfs in past selection criteria. We present photometric distance relations based on i - z and i - J colors and derive distances to our L dwarf sample. We combine the distances with SDSS/2MASS proper motions in order to examine the tangential velocities. For the majority of our spectroscopic sample, we measured radial velocities and present three-dimensional kinematics. We also provide Ha detections for the fraction of our sample with sufficient quality spectra. Comparison of the velocities of our L dwarf sample to a kinematic model shows evidence for both cold and hot dynamical populations, consistent with young and old disk components. The dispersions of these components are similar to those found for M dwarfs. We also show that J - K(S) color is correlated with velocity dispersion, confirming a relationship between J - K(S) color and age.
引用
收藏
页码:1808 / 1821
页数:14
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