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J/A+A/708/A136
  Effective supernova dust yield (Otaki+, 2026)
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2026A&A...708A.136O
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1.J/A+A/708/A136/tablea1Initial dust yields for non-rotating models (28 rows)
2.J/A+A/708/A136/tablea2Initial dust yields for rotating models (32 rows)
3.J/A+A/708/A136/tablea3Effective dust yields for non-rotating models with [Fe/H] = 0 (27 rows)
4.J/A+A/708/A136/tablea4Effective dust yields for non-rotating models with [Fe/H] = -1 (24 rows)
5.J/A+A/708/A136/tablea5Effective dust yields for non-rotating models with [Fe/H] = -2 (18 rows)
6.J/A+A/708/A136/tablea6Effective dust yields for non-rotating models with [Fe/H] = -3 (15 rows)
7.J/A+A/708/A136/tablea7Effective dust yields for rotating models with [Fe/H] = 0 (27 rows)
8.J/A+A/708/A136/tablea8Effective dust yields for rotating models with [Fe/H] = -1 (27 rows)
9.J/A+A/708/A136/tablea9Effective dust yields for rotating models with [Fe/H] = -2 (21 rows)
10.J/A+A/708/A136/tablea10Effective dust yields for rotating models with [Fe/H] = -3 (21 rows)

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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1+2)[Fe/H]   [-3/0] Initial metallicity (phys.abund.Z)
   (ALL)Mstar Msun Progenitor mass (13/15/20/25/30/40/60/80/120) (phys.mass)
   (ALL)Mdust Msun Total dust mass (phys.mass)
   (ALL)MAl2O3 Msun Al2O3 mass (phys.mass)
   (ALL)MFe Msun Fe mass (phys.mass)
   (ALL)MFe3O4 Msun Fe3O4 mass (phys.mass)
   (ALL)MMgSiO3 Msun MgSiO3 mass (phys.mass)
   (ALL)MMg2SiO4 Msun Mg2SiO4 mass (phys.mass)
   (ALL)MAC Msun AC mass (phys.mass)
   (ALL)MSiO2 Msun SiO2 mass (phys.mass)

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  (1+2)mu  Mean molecular weight (stat.weight)
  (3+4+5+6+7+8+9+10)eta % Surviving dust mass fraction (phys.mass;arith.ratio)
  (3+4+5+6+7+8+9+10)nISM cm-3 Interstellar medium density (phys.density)

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