VizieR

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

VizieR

  
J/MNRAS/500/1261
  Resolved molecular gas in nearby galaxies (Chown+, 2021)
ReadMe+ftp
2021MNRAS.500.1261C
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/500/1261/resolvedQuantities derived from spatially-resolved optical IFU and molecular gas maps (25321 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)
  ID   [0/25320] Pixel ID (meta.id)
  Name (char) Name of the galaxy that this pixel belongs to (meta.id;meta.main)
  fCO (char) [0/1] Flag indicating whether the CO measurement with the Simple method is a detection or an upper limit (Note 1)   (meta.code)
  bpt (char) BPT classification (Note 2)   (meta.code.class)
  Area kpc2 Area of the pixel (phys.area)
  12+logO/H [-] (n) Gas phase metallicity (phys.abund)
  alphaCO  (n) CO-to-H2 conversion factor from this metallicity αCO (arith.factor)
  f_logSM* (char) [*] Flag on logSM* (Note 3)   (meta.code)
  logSM* [Msun/pc2](n) Logarithm of the stellar mass surface density ΣM* (phys.density)
  logSSFR [Msun/yr/kpc2](n) Logarithm of the star formation rate surface density ΣSFR (phys.SFR)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  e_logSSFR [Msun/yr/kpc2](n) Error on logSSFR (stat.error)
  AV mag (n) Extinction measured from the Balmer decrement (phys.absorption)
  logLCO [K.pc2.km/s](n) Logarithm of the CO luminosity using the Sun method, including all pixels (phys.luminosity)
  e_logLCO [K.pc2.km/s](n) []? Error on logLCO (stat.error)
  logLCOsim [K.pc2.km/s](n) Logarithm of the CO luminosity using the Simple method, including all pixels (phys.luminosity)
  e_logLCOsim [K.pc2.km/s](n) []? Error on logLCOsim (stat.error)
  logSH2 [Msun/pc2](n) Logarithm of the H2 surface density using the Sun method, including all pixels, assuming αCO=3.2 (src.density)
  e_logSH2 [Msun/pc2](n) []? Error on logSH2 (stat.error)
  logSH2sim [Msun/pc2](n) Logarithm of the H2 surface density using the Simple method, including all pixels, assuming αCO=3.2 (src.density)
  e_logSH2sim [Msun/pc2](n) []? Error on logSH2sim (stat.error)
  logSH2amet [Msun/pc2](n) Logarithm of the H2 surface density using the Sun method, only star-forming pixels, assuming metallicity-dependent αCO (src.density)
  e_logSH2amet [Msun/pc2](n) []? Error on logSH2amet (stat.error)
  f_logL12 (char) [*] Flag on logL12 (Note 3)   (meta.code)
  logL12 [Lsun] (n) Logarithm of the 12µm luminosity (phys.luminosity;em.IR.8-15um)
  e_logL12 [Lsun] (n) []? Error on logL12 (stat.error)
  f_logS12 (char) [*] Flag on logS12 (Note 3)   (meta.code)
  logS12 [Lsun/pc2](n) Logarithm of the 12µm surface density (src.density)
  e_logS12 [Lsun/pc2](n) []? Error on logS12 (stat.error)

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