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J/A+A/664/A138
  Planet/star systems torque density distributions (Schib+, 2022)
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2022A&A...664A.138S
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1.J/A+A/664/A138/upp_1e-4Torque density distributions in a locally isothermal disk for various values of the planet-to-star mass ratio Mp/Ms=10–4 [timeSerie](torque density distribution)
timeSerie
(97 rows)
2.J/A+A/664/A138/upp_2e-4Torque density distributions in a locally isothermal disk for various values of the planet-to-star mass ratio Mp/Ms=2*10–4 [timeSerie](torque density distribution)
timeSerie
(57 rows)
3.J/A+A/664/A138/upp_3e-4Torque density distributions in a locally isothermal disk for various values of the planet-to-star mass ratio Mp/Ms=3*10–4 [timeSerie](torque density distribution)
timeSerie
(51 rows)
4.J/A+A/664/A138/upp_6e-5Torque density distributions in a locally isothermal disk for various values of the planet-to-star mass ratio Mp/Ms=6*10–5 [timeSerie](torque density distribution)
timeSerie
(82 rows)
5.J/A+A/664/A138/low_1e-3Torque density distributions in a locally isothermal disk for various values of the planet-to-star mass ratio Mp/Ms=10–3 [timeSerie](torque density distribution)
timeSerie
(91 rows)
6.J/A+A/664/A138/low_2e-3Torque density distributions in a locally isothermal disk for various values of the planet-to-star mass ratio Mp/Ms=2*10–3 [timeSerie](torque density distribution)
timeSerie
(101 rows)
7.J/A+A/664/A138/low_3e-4Torque density distributions in a locally isothermal disk for various values of the planet-to-star mass ratio Mp/Ms=3*10–4 [timeSerie](torque density distribution)
timeSerie
(62 rows)
8.J/A+A/664/A138/low_7e-4Torque density distributions in a locally isothermal disk for various values of the planet-to-star mass ratio Mp/Ms=7*10–4 [timeSerie](torque density distribution)
timeSerie
(76 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+3+4)(r-a)/H  Normalized radius, (r-a)/H (Note 1)   (phys.size.radius;arith.ratio)
   (ALL)dJ/dM  Magnitude of the torque densities, scaled by Ω2*a2(Mp/Ms)2(a/H)4 (stat.fit.param)
  (5+6+7+8)(r-a)/RH  Normalized radius, (r-a)/RH (Note 1)   (phys.size.radius;arith.ratio)

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