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  LMC eccentric ellipsoidal red giant binaries (Nicholls+, 2012)
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1.J/MNRAS/421/2616/solutionsSimultaneous light and velocity solutions for the 7 stars studied (50 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)
  ID (char) Number of the star as in table13 (
  i deg Inclination angle (src.orbital.inclination;pos.posAng)
  n_i (char) [abc] Final solution type (Note 1)   (meta.note)
  a Rsun Semi-major axis (phys.angSize.smajAxis;src.orbital)
  e_a Rsun rms uncertainty on a (stat.error)
  e  Eccentricity (src.orbital.eccentricity)
  e_e  rms uncertainty on e (stat.error)
  omega rad Angle of periastron ω (src.orbital.periastron)
  e_omega rad rms uncertainty on omega (stat.error)
  Omega1  Lagrangian potential of the primary Ω1 (arith.factor;phys.gravity)
  e_Omega1  rms uncertainty on Omega1 (stat.error)
  q  Mass ratio, M2/M1 (phys.mass)
  e_q  rms uncertainty on q (stat.error)
  M1 Msun Mass of the primary (phys.mass)
  M2 Msun Mass of the secondary (phys.mass)
  R1 Rsun Radius of the primary (phys.size.radius)
  Sum  Sum of squares of residuals of the I-band light curve from the modelled curve, Σ[r(I)]2 (

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