ZWCLUSTERS - Zwicky Clusters
Designation derived from the Zwicky cluster number. Cluster number (1...9134). This file is in ascending order by B1950.0 right ascension, whereas the original published catalogue is sorted by the survey field number and a running number within each survey field.
Right Ascension in 1950 Coordinates
Declination in 1950 Coordinates
The galactic longitude of the object.
The galactic latitude of the object.
Cluster types are 1 for open, 2 for medium compact, or 3 for compact.
The counted number of galaxies in the cluster.
The measured diameter of the cluster in centimeters.
Distance group, as estimated by Zwicky: 1 for near, 2 for medium distant, 3 for distant, 4 for very distant, or 5 for extremely distant.
Lambert coordinates. The Lambert tranformation is an equal-area projection. The Lambert distance RL from the nearest galactic pole is defined by RL = 2 sin ((90-b)/2), with RL > 0 for the north galactic hemisphere, and RL < 0 for the south galactic hemisphere.
Lambert coordinates. The X Lambert coordinate XL = 2 sin l sin ((90-b)/2).
Lambert coordinates. The Y Lambert coordinate YL = 2 cos l sin ((90-b)/2).
The supergalactic longitude of the object.
The supergalactic latitude of the object.
The cluster radius in degrees calculated as <clusrad> = 0.09326 * Diameter.
The cluster area in square degrees: 0.02733 * Diameter^2.
The mean apparent population (galaxies per square degree): population/area, taken from Cluster Pop and Cluster Area
The Right Ascension of the object.
The Declination of the object.
Right Ascension, Sexagesimal, J2000
Declination, Sexagesimal, J2000
BROWSE classification type.