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  Outer boundary conditions for evolving cool WD (Rohrmann+, 2012)
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1.J/A+A/546/A119/tableTemperature (T), pressure (P), geometrical depth (X), and stellar mass in outer layers, Mr/M (relative to the total stellar mass), for a Rosseland mean optical depth τ=25.11886 (logτ=1.4) (15621 rows)

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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Teff K [2000/40000] Effective temperature (phys.temperature.effective)
  log(g) [cm/s2] [5.5/9.5] Surface gravity acceleration (phys.gravity)
  log(T6) [10+6K] Temperature [106K] (phys.temperature)
  log(P15) [10+14Pa]Pressure [1015dyn/cm2] (phys.pressure)
  log(Mr/M) [---] Outer mass relative to the total stellar mass (phys.mass;arith.ratio)
  log(X) [10+8m] Geometrical depth [1010cm] (pos.distance)

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