Table 4.
Relationships between 
and β for the model galaxies evolved without galactic wind.
| log L = α * β + γ | ||||
|---|---|---|---|---|
| B-band |
V-band |
|||
| MB/M⊙ | α | γ | α | γ |
| 1e6 | –0.478 | 4.369 | –0.508 | 4.368 |
| 1e8 | –1.137 | 6.224 | –1.167 | 6.287 |
| 1e10 | –1.796 | 8.046 | –1.760 | 7.340 |
| 1e12 | –2.453 | 9.834 | –2.474 | 9.888 |
Notes. These relationships are the linear best fits of the curves shown in Fig. 24. All these relationships are nearly identical passing from models with large radii to those with smaller radii (by a factor of 4), and the corresponding solutions of the equations for β and 
, and finally changing only the photometric passband in use. The relationships seem to depend only on the galaxy mass.
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