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J/MNRAS/408/827
  Simulations of supernova explosions (Dessart+, 2010)
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2010MNRAS.408..827D
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1.J/MNRAS/408/827/table1Summary of the properties for a representative sample of pre-SN models employed in this study (9 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)
  Model (char) Pre-SN model designation (Note 1)   (meta.id;meta.main)
  Mi Msun Initial mass (i.e. the main-sequence mass) (phys.mass)
  Mf Msun Final mass (i.e. the mass at core collapse) (phys.mass)
  Mcore Msun Lagrangian mass delimiting outer edge of the core (phys.mass)
  MeO Msun Lagrangian mass delimiting outer edge of the oxygen (O) shell (phys.mass)
  MeHe Msun Lagrangian mass delimiting outer edge of the helium (He) shell (phys.mass)
  MiH Msun Lagrangian mass delimiting inner edge of the hydrogen (H) shell (phys.mass)
  MHenv Msun Mass of the hydrogen-rich envelope (phys.mass)
  DR 10+8km Size of the hydrogen-rich envelope (in 1013cm) (phys.size.radius)
  R* 10+8km surface radius (in 1013cm) (phys.size.radius)
  Egrav 10+44J Gravitational energy of the progenitor envelope outside of Mcore (in 1051erg) (phys.energy)
  Ebind 10+44J Binding energy of the progenitor envelope outside of Mcore (in 1051erg) (phys.energy)

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