Stellar mass distribution of S4G disk galaxies and signatures of bar-induced secular evolution

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Fig. 6

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Mean stellar mass density profiles for barred and non-barred disk galaxies (selected according to B2015 classification) and for weakly (B+SAB) and strongly (+SB) barred galaxies with 10^8.5 ≲ M_∗/M_⊙ ≲ 10¹¹ (90% sample coverage). Early-type (T< 5) and late-type (T ≥ 5) systems are studied separately.

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