AM 2

RA:

07 : 46.8

Dec:

-33 : 51

Distance from Sun:

kly

Distance from Galactic Center:

kly

Apparent Diameter:

arc min

Brightness:

mag vis

Radial Velocity:

Diameter:

Abs. Mag:

This object turned out to be most probably an open star cluster (Gratton and Ortolani, 1988).

References:

• R.G. Gratton and S. Ortolani, 1988. Astronomy and Astrophysics Supplement, Vol. 74, p. 299
• Barry F. Madore and Halton C. Arp, 1979. Three new faint star clusters. Astrophysical Journal, Vol. 227, p. L103-L104 and Plate L3-L6 (15 Jan 1979) [ADS: 1979ApJ...227L.103M]