Table 3
Fitted behavior of the effects of clumping and porosity when clumping sets in at the sonic point (model 2) and at 0.4 3∞ (model 3).
| D | 30 000 V | 40 000 V | 30 000 I | 40 000 I |
|
|
||||
| clumping sets in at the sonic point (model 2) | ||||
| 10 | –0.61 | –0.59 | –0.50 | –0.60 |
| 100 | –0.13 | –0.18 | –0.02 | –0.24 |
| 1000 | +0.11 | –0.02 | +0.17 | –0.11 |
| ∞ | +0.26 | +0.19 | +0.43 | +0.10 |
|
|
||||
| clumping sets in at 0.43∞ (model 3) | ||||
| 10 | –0.22 | –0.30 | –0.26 | –0.33 |
| 100 | +0.04 | –0.06 | +0.06 | –0.08 |
| 1000 | +0.19 | +0.08 | +0.20 | +0.03 |
| ∞ | +0.24 | +0.21 | +0.40 | +0.20 |
Notes. The total kinetic energy is fitted to the function Ekin = 
, for each type of star and clump separation L(r) = Hρ(r)/D. For given values of D, the table lists the values of α. D = ∞, corresponds to non-porous models
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