Table 13:
Best fit parameters for different isochrone fits to our observed
NGC 2451 colour-magnitude diagrams. Yale g and l denote two different
colour transformations (Green et al. 1987 and Lejeune et al. 1997), respectively.
Cluster |
Isochrone |
distance |
age |
|
|
(pc) |
(Myrs) |
NGC 2451 A |
Yale g |
201 |
80 |
NGC 2451 A |
Yale l |
201 |
80 |
NGC 2451 A |
Pols et al. |
206 |
63 |
NGC 2451 A |
Girardi et al. |
219 |
56 |
NGC 2451 B |
Yale g |
358 |
80 |
NGC 2451 B |
Yale l |
384 |
80 |
NGC 2451 B |
Pols et al. |
366 |
50 |
NGC 2451 B |
Girardi et al. |
380 |
63 |
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