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  Sub-mm clumps in Orion B South molecular cloud (Johnstone+, 2006)
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1.J/ApJ/639/259/clumpsClump properties in Orion South B molecular cloud (tables 1 and 2 of the paper) (57 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)
  SMMJ (char) Clump name (HHMMmm+DDMMm) (Note G1)   (;meta.main)
  RAJ2000 "h:m:s" (i) Hour of Right Ascension (J2000.0) (Note 1)   (pos.eq.ra;meta.main)
  DEJ2000 "d:m:s" (i) Degree of Declination (J2000.0) (Note 1)   (pos.eq.dec;meta.main)
  S850 Jy Total flux density at 850µm (Note 2)   (phot.flux.density;
  Sp850 Jy Peak flux at 850µm, in units of Jy/beam (Note 2)   (phot.flux.density;
  Reff 10+3AU Effective radius (Note 2)   (phys.size.radius)
  C  Degree of concentration (Note 3)   (meta.note)
  Td K Dust temperature (Note 3)   (phys.temperature)
  log(P/k) [K/cm+3] Bounding pressure (Note 3)   (phys.pressure)
  M1 solMass Mass derived from Bonnor-Ebert analysis (Note 3)   (phys.mass)
  M2 solMass Derived mass, assuming Td=20K (Note 4)   (phys.mass)
  FRt  Total flux ratio (S450um/S850um) (Note 1)   (phot.flux;arith.ratio)
  FRp  Peak flux ratio (Sp450um/Sp850um) (Note 1)   (phot.flux;arith.ratio)
  Td1 K Dust temperature derived from Bonnor-Ebert analysis (phys.temperature)
  Td2 K Dust temperature derived from spectral energy distribution (Note 2)   (phys.temperature)

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