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Table 4
Best power-law fits, 
, in which 
and 
, of the Lcor−M relations.
| Sample | Number | B | A | σlog 10L,intrinsic | B for A = 4/3 |
| of clusters | |||||
|
|
|||||
| Whole | 63 | −0.16 ± 0.06 | 1.29 ± 0.09 | 0.33 ± 0.04 | −0.18 ± 0.04 |
| Undisturbed | 39 | −0.14 ± 0.07 | 1.36 ± 0.13 | 0.39 ± 0.05 | −0.12 ± 0.06 |
| Disturbed | 24 | −0.29 ± 0.10 | 1.26 ± 0.14 | 0.22 ± 0.03 | −0.28 ± 0.05 |
| CC | 27 | + 0.02 ± 0.08 | 1.45 ± 0.16 | 0.41 ± 0.07 | −0.04 ± 0.08 |
| NCC | 36 | −0.27 ± 0.09 | 1.41 ± 0.13 | 0.23 ± 0.02 | −0.28 ± 0.04 |
|
|
|||||
| Whole (ngal ≥ 45) | 57 | −0.35 ± 0.05 | 1.44 ± 0.08 | 0.27 ± 0.02 | −0.24 ± 0.04 |
| Undisturbed (ngal ≥ 45) | 33 | −0.28 ± 0.06 | 1.57 ± 0.11 | 0.29 ± 0.03 | −0.21 ± 0.06 |
| CC (ngal ≥ 45) | 21 | −0.16 ± 0.07 | 1.66 ± 0.13 | 0.29 ± 0.06 | −0.16 ± 0.08 |
Notes. All disturbed clusters as well as NCC clusters have at least 45 member galaxies with spectroscopic redshifts per cluster in the current observational sample.
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