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  Orbits of 451 wide visual double stars (Izmailov, 2019)
Post annotation
1.J/PAZh/45/35/table3Sets of possible orbits, solution without weights (87844 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)
  WDS (char) WDS identifier (Cat. B/wds) (;meta.main)
  Disc (char) Discoverer & Number (
  Comp (char) Components (meta.code.multip)
  P yr Period (time.period)
  a arcsec Semi-major axis (a) (phys.angSize;src)
  i deg Inclination (i) (src.orbital.inclination)
  Omega deg Node (Omega) (src.orbital.node)
  T yr The time of periastron passage (T) in fractional Besselian year (src.orbital.periastron)
  e  Eccentricity (e) (src.orbital.eccentricity)
  omega deg Longitude of periastron (omega) (src.orbital.periastron)
  t0 yr epoch of the apparent motion parameters (time.epoch)
  rho0 arcsec Angular separation for t0 from orbit (pos.angDistance)
  theta0 deg Position angle for t0 from orbit (pos.posAng)
  pmrho arcsec/yrProper Motion (angular separation) for t0 from orbit (
  pmtheta deg/yr Proper Motion (position angle) for t0 from orbit (
  r arcsec Radius of curvature (phys.angSize)
  dVR arcsec/yrDifference between radial velocities for t0 from orbit (spect.dopplerVeloc;arith.diff)
  M Msun*arcsec+3Sum of mass of stars multiplied by parallax3 (phys.mass)

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