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J/MNRAS/462/1329
  Gas infall in disc galaxy models (Molla+, 2016)
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2016MNRAS.462.1329M
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1.J/MNRAS/462/1329/table1Characteristics of the theoretical galaxies modeled (Table 1 in the manuscript) (16 rows)

Simple ConstraintList Of Constraints
 
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  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  logMvir [Msun] The virial mass in logarithmic scale used as name for each galaxy (meta.id;meta.main)
  Mvir Msun The virial mass in the protohalo of each galaxy (phys.mass)
  MD Msun The barionic mass expected in the disk at the end of the evolution as obtained from the SHMR (phys.mass)
  MB Msun The bulge mass in each galaxy (phys.mass)
  Rvir kpc The virial radius for each galaxy at the end of the evolution (phys.size.radius)
  RD kpc The expected scale length of the disc at the end of the evolution (phys.angSize;src)
  Ropt kpc The expected optical radius of the disc at the end of the evolution (phys.angSize;src)
  Rcar kpc The characteristic radius of the disc used for normalization purposes (phys.size.radius)
  tauc Gyr The collapse time scale for the characteristic radius (time.scale)
  Vrot km/s The rotation velocity at the characteristic radius (phys.veloc.rotat)
  sigma0 km/s The dispersion velocity of the bulge (phys.veloc.dispersion)
  ReffB kpc The effective radius of the bulge (phys.size.radius)
  NR  Number of computed radial regions in each galaxy (meta.id;obs.field)

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