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  Variations on debris disks. II. (Kenyon+, 2010)
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1.J/ApJS/188/242/disksPredicted excesses for disks around stars of mass between 1 and 3M (tables 11-22 of paper) [model](plot of models) (1352 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)
  f (char) S for strong fragmentation parameters (produce more massive planets), W for weaker fragmentation parameters (produce produce planetesimals) (stat.param)
  p  (n)Exponent of a for Σ∝ap (stat.param)
  M solMass (n)Mass of central star (phys.mass)
  xm  Scaling factor (stat.param)
  logt [yr] Log time (Note 1)   (time.age)
  logLd [-] Log total dust/stellar luminosity ratio (phys.luminosity;arith.ratio)
  logF24 [-] Log of 24 micron flux excess (phot.flux.density;em.IR.15-30um)
  logF70 [-] Log of 70 micron flux excess (phot.flux.density;em.IR.30-60um)
  logF160 [-] Log of 160 micron flux excess (phot.flux.density;
  logF850 [-] Log of 850 micron flux excess (phot.flux.density;

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