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VII/110A/table6
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VII/110A
..table3
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Distance {rho}
Position angle {theta}
Distance (x,y)
Galactic
J2000
B1950
Ecl. J2000
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) or
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:
J2000
B1975
B1950
B1900
B1875
B1855
Galactic
Supergal.
Ecl.J2000
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deg
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arcsec
NB: The epoch used for the query is the original epoch of the table(s)
Radius
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VII/110A
14615
Rich Clusters of Galaxies (Abell+ 1989)
ReadMe+ftp
1989ApJS...70....1A
Similar Catalogs
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1.
VII/110A/table6
Overlap zone clusters
(274 rows)
meta
VII/110A/table6
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Constraint
Explain
(
UCD
)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
(unassigned);(unassigned);(unassigned);phys.veloc
)
(
RECORD
)
ABELL
[1,2712] "Abell" number for the clusters in the 10 deg overlap zone (-17 to -27 deg)
(
pos.galactic.lon;(unassigned);arith.diff;spect.line.veloc;arith
)
RAB1950
"h:m:s"
right ascension (B1950)
(
spect.index;(unassigned);arith.factor;(unassigned);arith
)
(
POS_EQ_RA_MAIN
)
DEB1950
"d:m:s"
declination (B1950)
(
(unassigned);(unassigned);(unassigned);(unassigned);arith
)
(
POS_EQ_DEC_MAIN
)
Field
(char)
[0-9F] the Southern Sky Survey Field number in which the cluster is located
(
(unassigned);stat.filling;arith.factor;spect.line.veloc;time.lifetime
)
Xcen
mm
rectangular coordinates if the apparent cluster center, referred to the CENTER of the Southern Sky Survey Field (+ = east)
(
(unassigned);phys.veloc.orbital;arith.diff;(unassigned);phys.atmol.term
)
Ycen
mm
same with above (+ = north)
(
(unassigned);(unassigned);(unassigned);(unassigned);phys.atmol.term
)
Atype
(char)
[ IR?:] cluster classification in Abell's system: I = irregular, R = regular, IR and RI = intermediate, ":" and "?" see file "
docu.txt
"
(
(unassigned);phys.veloc.orbital;arith.diff;phys.veloc.orbital
)
BMtype
(char)
[- I:?] cluster classification in the Bautz-Morgan system
(
(unassigned);(unassigned);(unassigned);phys.mass;meta.main
)
Count
ct
number of cluster members between m3 and m3+2, corrected for background
(
(unassigned);phys.veloc.orbital;arith.diff;src.var
)
u_Count
(char)
[:*?)] uncertainty of the Count
(
(unassigned);phys.veloc.orbital;arith.diff;pos.galactic.lon;time.duration
)
ALL
cols
(i)
indexed column
m1
mag
weighted mean total V mag. estimated for the first-ranked cluster member (no galactic extinction correction has been applied)
(
(unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned)
)
u_m1
(char)
[:?*] ":" = s.d. of more than ±0.5mag "?" = s.d. of more than ±1.0mag "*: = known or probable foreground object
(
(unassigned);(unassigned);(unassigned);pos.galactic.lon
)
m3
mag
weighted mean total V magnitude estimated for the third-ranked cluster member (again uncorrected)
(
(unassigned);em.IR.8-15um;arith.factor;stat.filling;(unassigned);(unassigned)
)
u_m3
(char)
[:?*] same with u_m1
(
(unassigned);(unassigned);(unassigned);pos.galactic.lon
)
m10
mag
weighted mean total V magnitude estimated for the tenth-ranked cluster member (again uncorrected)
(
(unassigned);(unassigned);(unassigned);stat.filling
)
u_m10
(char)
[:?*] same with u_m1
(
obs.param;(unassigned);(unassigned);pos.galactic.lon
)
Prev
(char)
[ BDdKOQRSs] sources of previous listings B = Braid and MacGillivray (
1978MNRAS.182..241B
), etc. see file "
docu.txt
"
(