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