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S.O. Kepler

Identifiers

  • name variant S.O. Kepler 0.60 · backfill

Papers (15)

  1. Asteroseismology of ZZ Ceti stars with full evolutionary white dwarf models. II. The impact of AGB thermal pulses on the asteroseismic inferences of ZZ Ceti stars astro-ph.SR · 2018 · author #5
  2. Low mass variable stars in the globular cluster NGC 6397 astro-ph.SR · 2017 · author #2
  3. White Dwarfs in the Metal-Rich Open Cluster NGC 6253 astro-ph.SR · 2016 · author #4
  4. DB white dwarfs in the Sloan Digital Sky Survey Data Release 10 and 12 astro-ph.SR · 2015 · author #2
  5. Extracting parameters from Colour-Magnitude Diagrams astro-ph.SR · 2015 · author #3
  6. New white dwarf stars in the Sloan Digital Sky Survey Data Release 10 astro-ph.SR · 2014 · author #1
  7. SDSS DR7 White Dwarf Catalog astro-ph.SR · 2012 · author #2
  8. Whole Earth Telescope Observations of the subdwarf B star KPD 1930+2752: A rich, short period pulsator in a close binary astro-ph.SR · 2010 · author #18
  9. SDSS White Dwarf mass distribution at low effective temperatures astro-ph · 2008 · author #2
  10. New Pulsating DB White Dwarf Stars from the Sloan Digital Sky Survey astro-ph · 2008 · author #4
  11. Pulsating White Dwarf Stars and Precision Asteroseismology astro-ph · 2008 · author #2
  12. Whole Earth Telescope observations of the hot helium atmosphere pulsating white dwarf EC 20058-5234 astro-ph · 2008 · author #8
  13. Whole Earth Telescope observations of BPM 37093: a seismological test of crystallization theory in white dwarfs astro-ph · 2004 · author #4
  14. The Everchanging Pulsating White Dwarf GD358 astro-ph · 2003 · author #1
  15. Mode identification of Pulsating White Dwarfs using the HST astro-ph · 2000 · author #1

Mentions

  • 1212.1222 #2 · backfill · confidence 0.70 S.O. Kepler
  • 1011.0387 #18 · backfill · confidence 0.70 S.O. Kepler
  • 0812.0491 #2 · backfill · confidence 0.70 S.O. Kepler
  • 0809.0921 #4 · backfill · confidence 0.70 S.O. Kepler
  • 0806.2573 #2 · backfill · confidence 0.70 S.O. Kepler
  • 0803.1638 #8 · backfill · confidence 0.70 S.O. Kepler

Frequent Coauthors