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Table 8.
Estimates of the probability density of the rotational velocity, P(ve), and its cumulative distribution function (cdf) for the NGC 346 apparently single B-type sample.
| ve | P(ve)×103 | cdf |
|---|---|---|
| 0 | 2.90 | 0.0000 |
| 20 | 2.90 | 0.0580 |
| 40 | 2.75 | 0.1145 |
| 60 | 2.40 | 0.1660 |
| 80 | 2.25 | 0.2125 |
| 100 | 2.20 | 0.2570 |
| 120 | 2.15 | 0.3005 |
| 140 | 2.15 | 0.3435 |
| 160 | 2.20 | 0.3870 |
| 180 | 2.25 | 0.4315 |
| 200 | 2.45 | 0.4785 |
| 220 | 2.60 | 0.5290 |
| 240 | 2.80 | 0.5830 |
| 260 | 2.95 | 0.6405 |
| 280 | 3.10 | 0.7010 |
| 300 | 3.60 | 0.7680 |
| 320 | 3.50 | 0.8390 |
| 340 | 2.55 | 0.8995 |
| 360 | 1.70 | 0.9420 |
| 380 | 1.00 | 0.9690 |
| 400 | 0.60 | 0.9850 |
| 420 | 0.25 | 0.9935 |
| 440 | 0.10 | 0.9970 |
| 460 | 0.05 | 0.9985 |
| 480 | 0.02 | 0.9992 |
| 500 | 0.00 | 0.9994 |
Notes. Supergiants (luminosity classes I and II) were excluded from the de-convolution.
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