Fig. 7.
Comparison between the g′ brightness profiles of the LSB galaxies detected in Pegasus I (black open squares with a dot) and those of six M 31 dSph satellites (Caldwell et al. 1992; Caldwell 1999). Andromeda’s satellites’ profiles were transformed from the V-band to the g′-band through the relations presented by Fukugita et al. (1995), and scaled to the distance of Pegasus I.
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