Properties of the Photometric Components of Lenticular Galaxies

Figure 13

Histograms of the distribution (a) and (c) and cumulative distribution (b) and (d) of bar strengths in S0 (dotted line) and spiral galaxies (full line). This figure shows that bars are weaker in S0 than in spiral galaxies. Credit: Buta et al. [190]. Reproduced by permission from the AAS.

(a)

(b)

(c)

(d)