VizieR

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J/A+A/560/A8
  STAGGER-grid of 3D stellar models. II. (Magic+, 2013)
model/atmosphere
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1.J/A+A/560/A8/staggerResults of the Stagger-grid for the 4 different reference depth scales (optical 500nm, column mass density, Rosseland, and geometrical height z) (14484 rows)

 
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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc)
  Teffi K [3935/7053] Effective temperature (input parameter) ((unassigned);(unassigned);(unassigned);em)
  loggi [cm/s2] [1.5/5] Surface gravity (input parameter) ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  [Fe/H]i [Sun] [-4/0.5] Metallicity (input parameter) ((unassigned);phys.veloc.orbital;arith.diff;phys.reflectance)
  Model (char) Model name (instr.fov;obs.atmos;arith.factor;spect.line.veloc;time.obs.end;src.orbital.meanAnomaly)
  logtau [-] [-5/2] log({tau}) ({tau} is the optical depth) ((unassigned);(unassigned);(unassigned);phys.particle.alpha)
  T(o) K Temperature at 500nm optical depth {tau} ((unassigned);(unassigned);(unassigned);em)
  rho(o) g/cm3 Density {rho} at 500nm optical depth {tau} ((unassigned);(unassigned);(unassigned);phys.particle.alpha)
  Pth(o) dPa Thermodynamic pressure [dyne/cm2] at {tau} ((unassigned);(unassigned);(unassigned);(unassigned))
  Ptb(o) dPa Turbulent pressure [dyne/cm2] at {tau} ((unassigned);pos.galactic.lon;arith.factor;(unassigned))
  Pe(o) dPa Electron pressure [dyne/cm2] at {tau} (time.lifetime;(unassigned);arith.factor;(unassigned))

ALL cols
    
 (i)indexed column
  T(m) K Temperature at Mean Rosseland optical depth {tau}, column mass density averaged ((unassigned);(unassigned);(unassigned);em)
  rho(m) g/cm3 Density {rho} at {tau} ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  Pth(m) dPa Thermodynamic pressure [dyne/cm2] at {tau} ((unassigned);(unassigned);(unassigned);(unassigned))
  Ptb(m) dPa Turbulent pressure [dyne/cm2] at {tau} ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  Pe(m) dPa Electron pressure [dyne/cm2] at {tau} ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  T(R) K Temperature at Rosseland optical depth {tau}, Rosseland optical depth averaged ((unassigned);phys.veloc.orbital;arith.diff;em)
  rho(R) g/cm3 Density {rho} at {tau} ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  Pth(R) dPa Thermodynamic pressure [dyne/cm2] at {tau} ((unassigned);(unassigned);(unassigned);(unassigned))
  Ptb(R) dPa Turbulent pressure [dyne/cm2] at {tau} ((unassigned);(unassigned);(unassigned);(unassigned))
  Pe(R) dPa Electron pressure [dyne/cm2] at {tau} ((unassigned);(unassigned);(unassigned);(unassigned))
  T(z) K Temperature at Mean Rosseland optical depth {tau}, geometrical height averaged ((unassigned);(unassigned);(unassigned);em)
  rho(z) g/cm3 Density {rho} at {tau} ((unassigned);(unassigned);(unassigned);(unassigned))
  Pth(z) dPa Thermodynamic pressure [dyne/cm2] at {tau} ((unassigned);(unassigned);(unassigned);pos.parallax;meta.main)
  Ptb(z) dPa Turbulent pressure [dyne/cm2] at {tau} ((unassigned);(unassigned);(unassigned);pos.parallax;meta.main)
  Pe(z) dPa Electron pressure [dyne/cm2] at {tau} ((unassigned);(unassigned);(unassigned);(unassigned))
  plot  Plot of T({tau}) (or density, pressure) ((unassigned);(unassigned);(unassigned);pos.geocentric)
model/atmosphere

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