Table 2: Here we show the values of χ for main sequence stars derived in the framework of the spectral variability method.
|
Spectral variability method: c for MSS |
||
|
Class |
T = 300 K |
T = 4000 K |
|
O |
> 0.59 |
~ (5.9 - 12) × 10-3 |
|
B |
~ 0.29 - 0.59 |
~ (2.9 - 5.9) × 10-3 |
|
A |
~ 0.24 - 0.29 |
~ (2.4 - 2.9) × 10-3 |
|
F |
~ 0.22 - 0.24 |
~ (2.2 - 2.4) × 10-3 |
|
G |
~ 0.2 - 0.22 |
~ (2 - 2.2) × 10-3 |
|
K |
~ 0.16 - 0.2 |
~ (1.6 - 2.2) × 10-3 |
|
M |
~ 0.1 - 0.16 |
~ (9 - 16) × 10-4 |