Table 5: $R_{\rm eff}/R_{\rm d}$ in UBVRI for the different Hubble types. This quotient decreases systematically from early to late spirals and decreases systematically from red to blue colors.
Hubble

Type I R V B U $\sigma$

1 0.701 0.626 0.550 0.475 0.399 0.204

2 0.491 0.432 0.373 0.314 0.256 0.125

3 0.264 0.239 0.214 0.189 0.164 0.084

4 0.146 0.132 0.117 0.103 0.089 0.053

5 0.153 0.130 0.108 0.085 0.063 0.051

**Table 5:** $R_{\rm eff}/R_{\rm d}$ in *UBVRI* for the different Hubble types. This quotient decreases systematically from early to late spirals and decreases systematically from red to blue colors.
Hubble
Type	I	R	V	B	U	$\sigma$
1	0.701	0.626	0.550	0.475	0.399	0.204
2	0.491	0.432	0.373	0.314	0.256	0.125
3	0.264	0.239	0.214	0.189	0.164	0.084
4	0.146	0.132	0.117	0.103	0.089	0.053
5	0.153	0.130	0.108	0.085	0.063	0.051

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