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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)

 
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)
  Teffi K [3935/7053] Effective temperature (input parameter) (phys.temperature)
  loggi [cm/s2] [1.5/5] Surface gravity (input parameter) (phys.gravity)
  [Fe/H]i [Sun] [-4/0.5] Metallicity (input parameter) (phys.abund.Fe)
  Model (char) Model name (meta.id;stat.param;meta.modelled)
  logtau [-] [-5/2] log(τ) (τ is the optical depth) (phys.absorption.opticalDepth)
  T(o) K Temperature at 500nm optical depth τ (phys.temperature)
  rho(o) g/cm3 Density ρ at 500nm optical depth τ (phys.absorption.opticalDepth)
  Pth(o) dPa Thermodynamic pressure [dyne/cm2] at τ (phys.pressure)
  Ptb(o) dPa Turbulent pressure [dyne/cm2] at τ (phys.pressure)
  Pe(o) dPa Electron pressure [dyne/cm2] at τ (phys.pressure)

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 K Temperature at Mean Rosseland optical depth τ, column mass density averaged (phys.temperature)
  rho(m) g/cm3 Density ρ at τ (phys.density)
  Pth(m) dPa Thermodynamic pressure [dyne/cm2] at τ (phys.pressure)
  Ptb(m) dPa Turbulent pressure [dyne/cm2] at τ (phys.pressure)
  Pe(m) dPa Electron pressure [dyne/cm2] at τ (phys.pressure)
  T(R) K Temperature at Rosseland optical depth τ, Rosseland optical depth averaged (phys.temperature)
  rho(R) g/cm3 Density ρ at τ (phys.density)
  Pth(R) dPa Thermodynamic pressure [dyne/cm2] at τ (phys.pressure)
  Ptb(R) dPa Turbulent pressure [dyne/cm2] at τ (phys.pressure)
  Pe(R) dPa Electron pressure [dyne/cm2] at τ (phys.pressure)
  T(z) K Temperature at Mean Rosseland optical depth τ, geometrical height averaged (phys.temperature)
  rho(z) g/cm3 Density ρ at τ (pjys.ddn{ity)
  Pth(z) dPa Thermodynamic pressure [dyne/cm2] at τ (src.redshift)
  Ptb(z) dPa Turbulent pressure [dyne/cm2] at τ (src.redshift)
  Pe(z) dPa Electron pressure [dyne/cm2] at τ (phys.pressure)
  plot  Plot of T(τ) (or density, pressure) (meta.ref.url)
model/atmosphere

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