VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/A+A/659/A135
  178 debris systems (Pearce+, 2022)
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2022A&A...659A.135P
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Post annotation 		img(gal)
1.J/A+A/659/A135/tablea2Planet and debris disc constraints calculated in this paper (178 rows)

Simple ConstraintList Of Constraints
 
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)
  System (char) System name (meta.id;meta.main)
  Mp Mjup Planet minimum mass that a single planet requires to sculpt the disc inner edge (phys.mass)
  E_Mp Mjup Error on Mp (upper value) (stat.error;stat.max)
  e_Mp Mjup Error on Mp (lower value) (stat.error)
  ap au Planet maximum semi-major axis that a single planet requires to sculpt the disc inner edge (phys.angSize;src)
  E_ap au Error on ap (upper value) (stat.error;stat.max)
  e_ap au Error on ap (lower value) (stat.error)
  ep  (n) Planet minimum eccentricity (Note 1)   (src.orbital.eccentricity)
  E_ep  (n) Error on ep (upper value) (stat.error;stat.max)
  e_ep  (n) Error on ep (lower value) (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  Qp arcsec Maximum apocentre distance that a single planet requires to sculpt the disc inner edge (src.orbital)
  E_Qp arcsec Error on Qp (upper limit) (stat.error;stat.max)
  e_Qp arcsec Error on Qp (lower limit) (stat.error)
  Mpn Mjup Minimum mass that each individual planet requires if instead multiple planets sculpt the disc inner edge (phys.mass)
  E_Mpn Mjup Error on Mpn (upper value) (stat.error;stat.max)
  e_Mpn Mjup Error on Mpn (lower value) (stat.error)
  rPn arcsec Maximum projected separation of the outermost planet in the multi-planet scenario (pos.angDistance;src.orbital)
  E_rPn arcsec Error on rPn (upper value) (stat.error;stat.max)
  e_rPn arcsec Error on rPn (lower value) (stat.error)
  Mpstir Mjup Minimum mass that a planet requires to stir the disc, assuming the planet eccentricity is ≤0.3 (phys.mass)
  E_Mpstir Mjup Error on Mpstir (upper value) (stat.error;stat.max)
  e_Mpstir Mjup (n) Error on Mpstir (lower value) (stat.error)
  Mdiscstir Mgeo (n) Minimum mass that the disc requires to self-stir (Note 2)   (phys.mass)
  E_Mdiscstir Mgeo (n) Error on Mdiscstir (upper value) (stat.error;stat.max)
  e_Mdiscstir Mgeo (n) Error on Mdiscstir (lower value) (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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