Multi-wavelength structure analysis of local cluster galaxies - The WINGS project

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Table 5.

The percentage changes of n and Re as shown in Figs. 13 and 15.

Morphological	(R_e(K)/R_e(u) – 1)×100	(R_e(K)/R_e(u) – 1)×100	(n(K)/n(u) – 1)×100	(n(K)/n(u) – 1)×100
class	cluster galaxies	non-member galaxies	cluster galaxies	non-member galaxies
Ellipticals	−44 ± 6	−31 ±13	−12 ± 5	−6 ± 10
S0s	−35 ± 9	−25 ±8	−1 ± 6	13 ± 10
Early-type spirals	−30 ± 21	−27 ±5	4 ± 15	20 ± 15
Late-type spirals	−40 ± 30	−27 ±8	19 ± 45	49 ± 33

Notes. The percentage changes of n and R_e from u- to K-band for cluster and non-member galaxies as presented in Figs. 13 and 15 (see Sect. 4.4.1 for more details of the formulas we used to calculate the percentage changes and their errors).

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