VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/A+A/335/823
  Evolution models of elliptical galaxies. III. (Tantalo+ 1998)
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1998A&A...335..823T
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1.J/A+A/335/823/table4Chemical Models at the Stage of Wind Ejection (66 rows)

Simple ConstraintList Of Constraints
 
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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  M(LT12) solMass Asymptotic mass M{L,T,12} (phys.mass)
  nu  Efficiency of star formation ν(rj/2) (stat.param)
  zeta  IMF parameter ζ (stat.fit.param)
  tau Gyr Time scale of mass accretion τ(rj/2) (time.scale)
  M(Lt) solMass Value reached by ML,t at the onset of galactic wind (phys.mass)
  Age Gyr Age at which the galactic wind occurs, tgω (time.age)
  G(rt)  Dimensionless mass of gas G(rj/2,t) (phys.mass;arith.ratio)
  S(rt)  Dimensionless mass of living stars S(rj/2,t) (phys.mass;arith.ratio)
  Zmax Sun Maximum metallicity, Z(rj/2,t) (phys.abund.Z)
  Zmean Sun Mean metallicity, <Z(rj/2,t)> (phys.abund.Z)
  Psi solMass/yrRate of star formation Ψ(rj/2,t) (phys.SFR)
  Omegag  Gravitational binding energy of the gas Ωg(rj/2,t) (phys.energy)
  Eg 10+43J Total thermal energy of this Eg(rj/2_,t) (phys.energy)
  ESNI 10+43J Contributions to the thermal energy by Type I supernovae (phys.energy)
  ESNII 10+43J Contributions to the thermal energy by Type II supernovae (phys.energy)
  ESW 10+43J Contributions to the thermal energy by stellar winds; (phys.energy)
  r  Mid shell fractionary radius rj/2 (phys.size.radius;arith.ratio)

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