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  Low-mass He-core white dwarfs seismic properties (Corsico+, 2012)
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1.J/A+A/547/A96/ava_g*Pulsation periods for g-modes with harmonic degree l=1 (Note) (44871 rows)

Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Mod   [1/95] Model number (Note 1)   (;
  M* Msun [0.16985/0.45219] Model stellar mass (Note G1)   (phys.mass)
  L* Lsun [0.0007347/0.12594] Model stellar luminosity (phys.luminosity)
  Teff K [7006.28/14223.5] Model effective temperature (phys.temperature.effective;meta.modelled)
  logMH/M* [-] [-3.44/-1.87] Model hydrogen mass in stellar mass units (phys.mass)
  Age Myr [11495.5/16446.7] Model age (time.age;meta.modelled)
  DPa s (n) Model asymptotic period spacing (for g-mode only) (time.period;meta.modelled)
  l   [1] Harmonic degree (
  k   [1/100] Radial order (
  Per s [0.501/5999.96] Pulsation period (time.period)
  DP s [-37.740/159.925] Period spacing (time.period)
  log(Ek) [10-7J] [38.8704/48.9739] Kinetic energy (
  Ckl   [-0.01261/0.88858] First order rotation splitting coefficient (

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