4.7 Article

New white dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 12

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv2526

关键词

catalogues; stars: magnetic field; subdwarfs; white dwarfs

资金

  1. CNPq-Brazil
  2. MCIT/MEC-Brazil
  3. German Aerospace Center (DLR) [05 OR 1507]
  4. Alfred P. Sloan Foundation
  5. National Science Foundation
  6. US Department of Energy Office of Science
  7. University of Arizona
  8. Brazilian Participation Group
  9. Brookhaven National Laboratory
  10. Carnegie Mellon University
  11. University of Florida
  12. French Participation Group
  13. German Participation Group
  14. Harvard University
  15. Instituto de Astrofisica de Canarias
  16. Michigan State/Notre Dame/JINA Participation Group
  17. Johns Hopkins University
  18. Lawrence Berkeley National Laboratory
  19. Max Planck Institute for Astrophysics
  20. Max Planck Institute for Extraterrestrial Physics
  21. New Mexico State University
  22. New York University
  23. Ohio State University
  24. Pennsylvania State University
  25. University of Portsmouth
  26. Princeton University
  27. Spanish Participation Group
  28. University of Tokyo
  29. University of Utah
  30. Vanderbilt University
  31. University of Virginia
  32. University of Washington
  33. Yale University

向作者/读者索取更多资源

We report the discovery of 6576 new spectroscopically confirmed white dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 12. We obtain T-eff, log g and mass for hydrogen atmosphere white dwarf stars (DAs) and helium atmosphere white dwarf stars (DBs), estimate the calcium/helium abundances for the white dwarf stars with metallic lines (DZs) and carbon/helium for carbon-dominated spectra (DQs). We found one central star of a planetary nebula, one ultracompact helium binary (AM CVn), one oxygen line-dominated white dwarf, 15 hot DO/PG1159s, 12 new cataclysmic variables, 36 magnetic white dwarf stars, 54 DQs, 115 helium-dominated white dwarfs, 148 white dwarf + main-sequence star binaries, 236 metal-polluted white dwarfs, 300 continuum spectra DCs, 230 hot subdwarfs, 2936 new hydrogen-dominated white dwarf stars, and 2675 cool hydrogen-dominated subdwarf stars. We calculate the mass distribution of all 5883 DAs with S/N >= 15 in DR12, including the ones in DR7 and DR10, with an average S/N = 26, corrected to the 3D convection scale, and also the distribution after correcting for the observed volume, using 1/Vmax.

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