Globular Cluster Palomar 13 (Pegasus Globular Cluster), class XII,
Discovered by A.G. Wilson in 1953.
- Distance from Sun:
- 84.8 kly
- Distance from Galactic Center:
- 87.7 kly
- Apparent Diameter:
- 2.2 arc min
- 13.47 mag vis
- Radial Velocity:
- +25.2 +/- 0.3 km/s
- Abs. Mag:
- -3.76 Mag vis
Palomar 13 was discovered by A.G. Wilson (1955) and
named by him the Pegasus Globular Cluster, together with globular clusters
Palomar 3, Palomar 4
and Palomar 5, and two new Local Group galaxies.
That naming was certainly not essentially a happy choice, as Pegasus also
contains the prominent globular M15.
G.O. Abell (1955) cataloged them with their Palomar
- 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)
- A.G. Wilson, 1955.
Sculptor-Type Systems in the Local Group of Galaxies.
Publications of the Astronomical Society of the Pacific, Vol. 67, No. 394,
pp. 27-29 (02/1955)
[MW Globulars] |