Fig. 1. V-band image of the IBm galaxy UGCA 65 taken with the CTIO 1.5 m telescope by Gallagher & L.D. Matthews. This system is at a distance of ≅ 18 Mpc and has M_B ≅ -15.5

Fig. 2. Map of the LMC based on star counts derived from the USNO-A1.0 catalog. The off-center bar and symmetric outer disk are easily seen (orientation: N to right). This map was produced by S. Levine (private communication)

Fig. 3. V band image of the central regions of the Local Group dE NGC 147 taken with the WIYN 3.5 m telescope. The distribution of red giant branch stars, resolved in this image with sub-arcsecond seeing, give dEs their characteristic smooth structures