Segue 1

Globular Cluster Candidate Segue 1, actually Local Group dSph galaxy, in Leo

RA:
10:07:04
Dec:
+12:47:30
Distance from Sun:
75.0 kly
Distance from Galactic Center:
Apparent Diameter:
4.5 arc min
Brightness:
14.7 mag (vis)
Radial Velocity:
Diameter:
c. 10 ly
Abs. Mag:
c. -2

Discovered by Belokurov et.al. 2006 in the SDSS imaging data.

Discovered in 2006 (Belokurov et.al. 2007), this object was considered a Globular Cluster candidate by Harris (2010), but is now thought to be a dwarf spheroidal galaxy in the Local Group, a satellite of the Milky Way.

.. more to come ..

References:



[MW Globulars] | [DSS] | [SIMBAD] | [ADS] | [GGC-DB]
Hartmut Frommert [contact]
[SEDS]