4.6 Article

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

Journal

ASTRONOMICAL JOURNAL
Volume 139, Issue 5, Pages 1808-1821

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/139/5/1808

Keywords

brown dwarfs; solar neighborhood; stars: kinematics and dynamics; stars: low-mass

Funding

  1. National Science Foundation (NSF) [AST 06-07644]
  2. National Aeronautics and Space Administration
  3. Alfred P. Sloan Foundation
  4. American Museum of Natural History
  5. Astrophysical Institute Potsdam
  6. University of Basel
  7. University of Cambridge
  8. Case Western Reserve University
  9. University of Chicago
  10. Drexel University
  11. Fermilab
  12. Institute for Advanced Study
  13. Japan Participation Group
  14. Johns Hopkins University
  15. Joint Institute for Nuclear Astrophysics
  16. Kavli Institute for Particle Astrophysics and Cosmology
  17. Korean Scientist Group
  18. Chinese Academy of Sciences (LAMOST)
  19. Los Alamos National Laboratory
  20. Max-Planck-Institute for Astronomy (MPIA)
  21. Max-Planck-Institute for Astrophysics (MPA)
  22. New Mexico State University
  23. Ohio State University
  24. University of Pittsburgh
  25. University of Portsmouth
  26. Princeton University
  27. United States Naval Observatory
  28. University of Washington
  29. Division Of Astronomical Sciences
  30. Direct For Mathematical & Physical Scien [0909463] Funding Source: National Science Foundation

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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.

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