VizieR

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

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
 Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/AJ/160/66
  LITTLE THINGS catalog of HI holes in 41 galaxies (Pokhrel+, 2020)
ReadMe+ftp
2020AJ....160...66P
Similar Catalogs
Post annotation 		img(gal)
1.J/AJ/160/66/holesHoles properties (merge of all tables from Appendix B) (306 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)
  Gal (char) Identification of the galaxy (meta.id.parent)
  Seq  Hole sequential identification (meta.id;meta.main)
  RAJ2000 "h:m:s" (i) Hour of right ascension (J2000) (pos.eq.ra;meta.main)
  DEJ2000 "d:m:s" (i) Degree of declination (J2000) (pos.eq.dec;meta.main)
  vhel km/s Heliocentric velocity (phys.veloc;pos.heliocentric)
  vexp km/s Expansion velocity (phys.veloc.expansion)
  Type  Hole type (src.class)
  PA deg Position angle (pos.posAng)
  Diam pc Hole's diameter (pos.distance)
  Age Myr Age (time.age)
  logNHI [/cm2] Log H I column density (1020/cm–2) (phys.columnDensity)
  Rad kpc Radius (phys.size.radius)
  b/a  Axial ratio (phys.angSize;arith.ratio)
  Mass Msun (n) H I mass (104M☉) (phys.mass)
  logEMc [10-7J] (n) Energy required to form the hole calculated with McCray method (1050erg) (Note 1)   (phys.energy)
  logECh [10-7J] (n) Energy required to form the hole calculated with Chevalier method (1050erg) (Note 2)   (phys.energy)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
Adapt form
 Display your selection only Reset to default columns
usage  Display UCD1+    UCD1  
elapse time 0
→ Cite/acknowledge VizieR catalogue
→ Rules of usage of VizieR data

© UDS/CNRS

Contact