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VI/156
  M-dwarf Lum-Temp-Radius relationships (Morrell+, 2019)
ReadMe+ftp
2019MNRAS.489.2615M
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Post annotation 		img(gal)
1.VI/156/table4Tabulated form of our LSED-R relation for M-dwarf stars (corrected version) (98 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)
  LSED Lsun [0.0/0.1] Luminosity of the source from a SED fit (lsed) (phys.luminosity)
  Radcorr Rsun [0.0/0.7] Radius correction to the D08 4Gyr isochrone at luminosity LSED (radius_correction) (arith.factor;phys.size.radius)
  b_Radcorr Rsun [-0.1/0.7] Lower bound radius correction to the D08 4Gyr isochrone at luminosity LSED (radiuscorrectionlbound) (arith.factor;phys.size.radius;stat.min)
  B_Radcorr Rsun [0.0/0.7] Upper bound radius correction to the D08 4Gyr isochrone at luminosity LSED (radiuscorrectionubound_ (arith.factor;phys.size.radius;stat.max)
  Rad Rsun [0.1/0.7] Radius prescribed by the relation at luminosity LSED (radius) (phys.size.radius)
  b_Rad Rsun [0.1/0.7] Lower bound radius prescribed by the relation at luminosity LSED (radius_lbound) (phys.size.radius;stat.min)
  B_Rad Rsun [0.2/0.8] Upper bound radius prescribed by the relation at luminosity LSED (radius_ubound) (phys.size.radius;stat.max)

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