Palomar 2
Globular Cluster Palomar 2, class IX,
in Auriga
- RA:
- 04:46:05.9
- Dec:
- +31:22:51
- Distance from Sun:
- 90.0 kly
- Distance from Galactic Center:
- 115.5 kly
- Apparent Diameter:
- 1.9 arc min
- Brightness:
- 13.04 mag vis
- Radial Velocity:
-
- Diameter:
-
- Abs. Mag:
-
Discovered by A.G. Wilson in 1955.
Links:
References:
- George O. Abell, 1955.
Globular Clusters and Planetary Nebulae Discovered on the National Geographic
Society-Palomar Observatory Sky Survey.
Publications of the Astronomical Society of the Pacific, Vol. 67, No. 397,
p. 258 (August 1955)
- W.E. Harris, P.R. Durrell, G.R. Petitpas, T.M. Webb and
S.C. Woodworth, 1997.
Unveiling Palomar 2: The most obscure globular cluster in the outer halo.
Astronomical Journal, Vol. 114, p. 1043-1050 (09/1997)
[MW Globulars] |
[DSS] |
[SIMBAD] |
[ADS] |
[GGC-DB]
Hartmut Frommert
[contact]
[SEDS]