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  Abundance ratio in gamma-ray burst (Contini, 2017)
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1.J/MNRAS/469/3125/table6Models used to reproduce the spectra presented in Table 5 (28 rows)

Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Model (char) Model name (;stat.param;meta.modelled)
  Vs km/s Shock velocity (phys.veloc)
  n0 cm-3 Atomic pre-shock density (phys.density)
  F 10+10ph/cm2/s/eVFlux at the Lyman limit (phot.flux;em.UV)
  D 10+17cm Geometrical thickness (src.morph.param)
  N/H 10-4 N/H relative abundance (phys.abund)
  O/H 10-4 O/H relative abundance (phys.abund)
  S/H 10-4 S/H relative abundance (phys.abund)
  FHb mW/m2 Bβ flux, calculated at the nebula (in erg/cm2/s) (phot.flux;em.line.Hbeta)

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